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description Publicationkeyboard_double_arrow_right Preprint , Article 2021 FrancePublisher:EDP Sciences Publicly fundedQuentin Kral; J. E. Pringle; A. Guilbert-Lepoutre; Luca Matrà; Julianne I. Moses; Emmanuel Lellouch; Mark C. Wyatt; N. Biver; Dominique Bockelée-Morvan; Amy Bonsor; F. Le Petit; G. Randall Gladstone;Gas has been detected in many exoplanetary systems ($>$10 Myr), thought to be released in the destruction of volatile-rich planetesimals orbiting in exo-Kuiper belts. In this letter, we aim to explore whether gas is also expected in the Kuiper belt (KB) in our Solar System. To quantify the gas release in our Solar System, we use models for gas release that have been applied to extrasolar planetary systems, as well as a physical model that accounts for gas released due to the progressive internal warming of large planetesimals. We find that only bodies larger than about 4 km can still contain CO ice after 4.6 Gyr of evolution. This finding may provide a clue as to why Jupiter-family comets, thought to originate in the Kuiper belt, are deficient in CO compared to Oort-clouds comets. We predict that gas is still produced in the KB right now at a rate of $2 \times 10^{-8}$ M$_\oplus$/Myr for CO and orders of magnitude more when the Sun was younger. Once released, the gas is quickly pushed out by the Solar wind. Therefore, we predict a gas wind in our Solar System starting at the KB location and extending far beyond with regards to the heliosphere with a current total CO mass of $\sim 2 \times 10^{-12}$ M$_\oplus$. We also predict the existence of a slightly more massive atomic gas wind made of carbon and oxygen (neutral and ionized) with a mass of $\sim 10^{-11}$ M$_\oplus$. We predict that gas is currently present in our Solar System beyond the Kuiper belt and that although it cannot be detected with current instrumentation, it could be observed in the future with an in situ mission using an instrument similar to Alice on New Horizons with larger detectors. Our model of gas release due to slow heating may also work for exoplanetary systems and provide the first real physical mechanism for the gas observations. accepted for publication as a Letter to the editor in A&A; abstract shortened; 15 pages, 5 figures, 4 tables
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/202141783&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 6 citations 6 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/202141783&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Preprint 2021 Switzerland, France, France, Netherlands, Germany, France, PolandPublisher:Sissa Medialab Funded by:IRCIRCAlison Mitchell; Sami Caroff; Jim Hinton; L. Mohrmann; Felix Aharonian; Faical Ait-Benkhali; Oguzhan Anguener; C. Arcaro; Celine Armand; Tom Armstrong; Halim Ashkar; Michael Backes; Vardan Baghmanyan; Victor Barbosa Martins; Anna Barnacka; Monica Barnard; Rowan Batzofin; David Berge; K. Bernloehr; B. Bi; Markus Boettcher; Catherine Boisson; J. Bolmont; Mathieu Bony; Mischa Breuhaus; Robert Brose; Francois Brun; Tomasz Bulik; Floriane Cangemi; Sabrina Casanova; Jaqueline Catalano; Pauline Chambery; T. Chand; A. W. Chen; Garret Cotter; Malgorzata Curlo; Hannah Dalgleish; Jean Damascene Mbarubucyeye; Isak Delberth Davids; James Davies; Justine Devin; Arache Djannati-Ataï; Anton Dmytriiev; Axel Donath; Victor Doroshenko; Lente Dreyer; Kathrin Egberts; Sabrina Einecke; Jean-Pierre Ernenwein; S. J. Fegan; Kirsty Feijen; A. Fiasson; Lott Frans; Stefano Gabici; Yves Gallant; Gianluca Giavitto; L. Giunti; Dorit Glawion; J. F. Glicenstein; M.-H. Grondin; Sumari Hattingh; Maria Haupt; German Hermann; Werner Hofmann; Clemens Hoischen; Tim Holch; Markus Holler; Zhiqiu Huang; David Huber; M. Hörbe; Marek Jamrozy; Felix Jankowsky; Vikas Joshi; Ira Jung; E. Kasai; Krzysztof Katarzynski; U. Katz; Dmitry Khangulyan; Bruno Khelifi; Stefan Klepser; Wlodek Kluzniak; R. Konno; K. Kosack; Dmitriy Kostunin; Michael Kreter; Gašper Kukec Mezek; Anu Kundu; Sébastien Le Stum; M. Lemoine-Goumard; J.-P. Lenain; Fabian Leuschner; C. Levy; Thomas Lohse; Anna Luashvili; Iryna Lypova; Jonathan Mackey; Jhilik Majumdar; D. Malyshev; Vincent Marandon; Paolo Marchegiani; Guillem Marti'i-Devesa; Ramin Marx; Gilles Maurin; P. J. Meintjes; Manuel Meyer; Rafal Moderski; Alessandro Montanari; C. Moore; Paul Morris; Emmanuel Moulin; Jacques Muller; Thomas Murach; Mathieu Naurois; Amid Nayerhoda; Hambeleleni Ndiyavala; Jacek Niemiec; Angel Noel; P. T. O'Brien; Laenita Lorraine Oberholzer; Stefan Ohm; Laura Olivera-Nieto; Michal Ostrowski; Sebastian Panny; M. Panter; Dan Parsons; G. Peron; Santiago Pita; V. Poireau; D. A. Prokhorov; Heike Prokoph; Gerd Puehlhofer; Michael Punch; Andreas Quirrenbach; P. Reichherzer; Anita Reimer; Olaf Reimer; Q. Remy; Matthieu Renaud; Frank M. Rieger; Carlo Romoli; Gavin Rowell; B. Rudak; Edna Ruiz Velasco; V. Sahakian; S. Sailer; David Sanchez; Andrea Santangelo; Manami Sasaki; Johannes Schaefer; Hester Schutte; Ullrich Schwanke; Fabian Schüssler; Mohanraj Senniappan; Albert Seyffert; Jimmy N.S. Shapopi; Rachel Simoni; Atreyee Sinha; Helene Sol; Andreas Specovius; Samuel Timothy Spencer; Marion Spir-Jacob; Lukasz Stawarz; Riaan Steenkamp; Christian Stegmann; S. Steinmassl; Constantin Steppa; Lei Sun; Tadayuki Takahashi; Takaaki Tanaka; Thomas Tavernier; Andrew Taylor; Regis Terrier; Hannes Thiersen; Charles Thorpe-Morgan; Martin Tluczykont; Lenka Tomankova; Michelle Tsirou; Naomi Tsuji; R. J. Tuffs; Yasunobu Uchiyama; Johann van der Walt; Christopher van Eldik; Carlo van Rensburg; Brian van Soelen; G. Vasileiadis; Johannes Veh; Jacco Vink; Heinrich J. Völk; Stefan Wagner; Jason John Watson; Felix Werner; Richard White; Alicja Wierzcholska; Yu Wun Wong; A. Yusafzai; Roberta Zanin; Davit Zargaryan; A. A. Zdziarski; Andreas Zech; Sylvia Zhu; Andreas Zmija; N. Zywucka;Highly extended gamma-ray emission around the Geminga pulsar was discovered by Milagro and verified by HAWC. Despite many observations with Imaging Atmospheric Cherenkov Telescopes (IACTs), detection of gamma-ray emission on angular scales exceeding the IACT field-of-view has proven challenging. Recent developments in analysis techniques have enabled the detection of significant emission around Geminga in archival data with H.E.S.S.. In 2019, further data on the Geminga region were obtained with an adapted observation strategy. Following the announcement of the detection of significant TeV emission around Geminga in archival data, in this contribution we present the detection in an independent dataset. New analysis results will be presented, and emphasis given to the technical challenges involved in observations of highly extended gamma-ray emission with IACTs. Proceedings of 37th International Cosmic Ray Conference PoS: Proceedings of Science, 395 ISSN:1824-8039
MPG.PuRe arrow_drop_down Digitala Vetenskapliga Arkivet - Academic Archive On-lineArticle . 2023 . Peer-reviewedJagiellonian University RepositoryConference object . 2022Data sources: Jagiellonian University RepositoryHAL AMU; Mémoires en Sciences de l'Information et de la Communication; HAL-CEAArticle . 2023License: CC BYFull-Text: https://hal.science/hal-04080197/documentMémoires en Sciences de l'Information et de la CommunicationConference object . 2021add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.22323/1.395.0780&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 8 citations 8 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert MPG.PuRe arrow_drop_down Digitala Vetenskapliga Arkivet - Academic Archive On-lineArticle . 2023 . Peer-reviewedJagiellonian University RepositoryConference object . 2022Data sources: Jagiellonian University RepositoryHAL AMU; Mémoires en Sciences de l'Information et de la Communication; HAL-CEAArticle . 2023License: CC BYFull-Text: https://hal.science/hal-04080197/documentMémoires en Sciences de l'Information et de la CommunicationConference object . 2021add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.22323/1.395.0780&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2021 France, ItalyPublisher:Wiley Godard M.; Carter E. J.; Decrausaz T.; Lafay R.; Bennett E.; Kourim F.; Obeso J. ‐C.; Michibayashi K.; Harris M.; Coggon J. A.; Teagle D. A. H.; Kelemen P. B.; the Oman Drilling Project Phase 1 Science Party (include Laura Crispini); L. Crispini;handle: 11567/1067756
AbstractThe transition from the Semail ophiolite mantle to the underlying metamorphic sole was drilled at ICDP OmanDP Hole BT1B. We analyzed the bulk major, volatile and trace element compositions of the mantle‐derived listvenite series and metamorphic rocks, with the aim to constrain chemical transfers associated with peridotite carbonation along the ophiolite basal thrust. The listvenite series comprise variously carbonated serpentinites and (fuchsite‐bearing) listvenites. They have high CO2 (up to 43 wt.%) and variable H2O (0–12 wt.%). Yet, they have compositions close to that of the basal banded peridotites for most major and lithophile trace elements, with fuchsite‐bearing listvenites overlapping in composition with amphibole‐bearing basal lherzolites (e.g., Al2O3 = 0.1–2.2 wt.%; Yb = 0.05–1 x CI‐chondrite). The protolith of the listvenite series was likely similar in structure and composition to serpentinized banded peridotites which immediately overlie the metamorphic sole elsewhere in Oman. The listvenite series are enriched in fluid mobile elements (FME) compared to Semail peridotites (up to ∼103–104 x Primitive Mantle), with concentrations similar to the underthrusted metabasalts and/or metasediments for Cs, Sr and Ca and sometimes even higher for Pb, Li, As, and Sb (e.g., Li up to 130 μg/g; As up to 170 μg/g). We also observe a decoupling between Sr‐Ca enrichments and other FME, indicating interactions with several batches of deep CO2‐rich fluids transported along the basal thrust. These results suggest that peridotite carbonation could represent one of the major trap‐and‐release mechanisms for carbon, water and FME along convergent margins.
https://hal.archives... arrow_drop_down Journal of Geophysical Research Solid EarthArticle . 2021 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2021Full-Text: https://hal.science/hal-03501317/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/essoar.10507497.1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu4 citations 4 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert https://hal.archives... arrow_drop_down Journal of Geophysical Research Solid EarthArticle . 2021 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2021Full-Text: https://hal.science/hal-03501317/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/essoar.10507497.1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2021 FrancePublisher:Wiley Publicly fundedCorentin Louis; Ph. Zarka; K. Dabidin; P.-A. Lampson; F. P. Magalhães; A. Boudouma; M. S. Marques; Baptiste Cecconi;AbstractThe observations from the Juno spacecraft in polar orbit of Jupiter provide for the first time a complete view of Jupiter's radio emissions from all latitudes. Characterizing the latitudinal distribution of radio emissions' occurrence and intensity is a useful step for elucidating their origin. Here, we analyze for that purpose the first 3 years of observations from the Waves experiment on the Juno spacecraft (mid‐2016 to mid‐2019). Two prerequisites for the construction of the latitudinal distribution of intensities for each Jovian radio component are (a) to work with absolute flux densities and (b) to be able to associate each radio measurement with a specific radio component. Accordingly, we develop a method to convert the Juno/Waves data in flux densities and then we build a catalog of all Jovian radio components over the first 3 years of Juno's orbital mission. From these, we derive occurrence and intensity distributions versus observer's latitude and frequency for each component; these will be the basis for future detailed studies and interpretations of each component's characteristics and origin.
Journal of Geophysic... arrow_drop_down Journal of Geophysical Research Space PhysicsArticle . 2021 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2021Full-Text: https://hal.science/hal-03368294/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/essoar.10506795.1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 4 citations 4 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Journal of Geophysic... arrow_drop_down Journal of Geophysical Research Space PhysicsArticle . 2021 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2021Full-Text: https://hal.science/hal-03368294/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/essoar.10506795.1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2021 France, United Kingdom, FrancePublisher:Oxford University Press (OUP) Publicly fundedFunded by:IRC, EC | NewWorlds, EC | GPRV +2 projectsIRC ,EC| NewWorlds ,EC| GPRV ,EC| ASTROFLOW ,UKRI| Astronomy at St Andrews 2018-2021Robert D. Kavanagh; Aline A. Vidotto; Baptiste Klein; Moira Jardine; Jean-François Donati; Dúalta Ó Fionnagáin;handle: 10023/23042
There have recently been detections of radio emission from low-mass stars, some of which are indicative of star-planet interactions. Motivated by these exciting new results, in this paper we present Alfv\'en wave-driven stellar wind models of the two active planet-hosting M dwarfs Prox Cen and AU Mic. Our models incorporate large-scale photospheric magnetic field maps reconstructed using the Zeeman-Doppler Imaging method. We obtain a mass-loss rate of $0.25~\dot{M}_{\odot}$ for the wind of Prox Cen. For the young dwarf AU Mic, we explore two cases: a low and high mass-loss rate. Depending on the properties of the Alfv\'en waves which heat the corona in our wind models, we obtain mass-loss rates of $27$ and $590~\dot{M}_{\odot}$ for AU Mic. We use our stellar wind models to assess the generation of electron cyclotron maser instability emission in both systems, through a mechanism analogous to the sub-Alfv\'enic Jupiter-Io interaction. For Prox Cen we do not find any feasible scenario where the planet can induce radio emission in the star's corona, as the planet orbits too far from the star in the super-Alfv\'enic regime. However, in the case that AU Mic has a stellar wind mass-loss rate of $27~\dot{M}_{\odot}$, we find that both planets b and c in the system can induce radio emission from $\sim10$ MHz to 3 GHz in the corona of the host star for the majority of their orbits, with peak flux densities of $\sim10$ mJy. Detection of such radio emission would allow us to place an upper limit on the mass-loss rate of the star. Comment: 8 pages, 5 figures. Accepted for publication in MNRAS
Monthly Notices of t... arrow_drop_down Monthly Notices of the Royal Astronomical SocietyOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYSt Andrews Research RepositoryArticle . 2021 . Peer-reviewedData sources: St Andrews Research Repositoryhttps://doi.org/10.48550/arxiv...Article . 2021License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1093/mnras/stab929&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 35 citations 35 popularity Top 1% influence Average impulse Top 10% Powered by BIP!visibility 3visibility views 3 download downloads 13 Powered bymore_vert Monthly Notices of t... arrow_drop_down Monthly Notices of the Royal Astronomical SocietyOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYSt Andrews Research RepositoryArticle . 2021 . Peer-reviewedData sources: St Andrews Research Repositoryhttps://doi.org/10.48550/arxiv...Article . 2021License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1093/mnras/stab929&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2021 Germany, Denmark, Italy, Italy, Netherlands, Italy, Italy, Spain, Netherlands, Italy, Netherlands, Croatia, Italy, United States, Germany, France, Finland, Italy, Italy, Netherlands, Netherlands, Italy, Croatia, Netherlands, Poland, Netherlands, Italy, France, Bulgaria, France, FrancePublisher:American Astronomical Society Publicly fundedFunded by:EC | RadioNet, NSF | Collaborative Research: B..., AKA | Physics of Black Hole-Pow... +17 projectsEC| RadioNet ,NSF| Collaborative Research: Building an Event Horizon Telescope: (Sub)millimeter VLBI from the South Pole Telescope ,AKA| Physics of Black Hole-Powered Jets ,EC| PROBIST ,NSERC ,NSF| Graduate Research Fellowship Program (GRFP) ,NWO| From micro- to mega-scales: understanding how black holes shape the local Universe ,NSF| CyVerse: Cyberinfrastructure for the Life Sciences ,NSF| Physics Frontier Center at the Kavli Institute for Cosmological Physics: Pushing Cosmology to the Edge ,NSF| The Arizona Radio Observatory: Surveying the ISM through Millimeter and Sub-millimeter Spectroscopy ,NSF| The iPlant Collaborative: Cyberinfrastructure for the Life Sciences ,EC| BLACKHOLECAM ,AKA| Physics of Black Hole-Powered Jets ,NSF| PSCIC Full Proposal: The iPlant Collaborative: A Cyberinfrastructure-Centered Community for a New Plant Biology ,AKA| Physics of Black Hole-Powered Jets ,AKA| Intrinsic Very High Energy Gamma-ray Emission of Blazars ,NSF| Cosmological Research with the 10-meter South Pole Telescope ,HRZZ| Very high energy gamma-ray astronomy with the MAGIC and CTA telescopes ,AKA| From quasars to geodesy: how astronomy can enable a new era in ultra-precise geodetic measurements / Consortium: NT-VGOS ,NSF| Collaborative Research: Building an Event Horizon Telescope: (Sub)millimeter VLBI from the South Pole TelescopeJuan-Carlos Algaba; Jadyn Anczarski; Keiichi Asada; M. Balokovic; S. Chandra; Yuzhu Cui; A. D. Falcone; Marcello Giroletti; Ciriaco Goddi; Kazuhiro Hada; Daryl Haggard; Tomohisa Kawashima; Garrett K. Keating; Motoki Kino; S. Komossa; E. V. Kravchenko; Sera Markoff; J. Neilsen; Jongho Park; G. Principe; V. Ramakrishnan; Mahito Sasada; Kazunori Akiyama; Antxon Alberdi; Richard Anantua; Rebecca Azulay; Anne Kathrin Baczko; David Ball; Bradford Benson; Lindy Blackburn; Raymond Blundell; Katherine L. Bouman; Geoffrey C. Bower; Hope Boyce; Christiaan D. Brinkerink; Roger Brissenden; Silke Britzen; Avery E. Broderick; Dominique Broguiere; Thomas Bronzwaer; Do-Young Byun; Andrew Chael; Chi-kwan Chan; Shami Chatterjee; Koushik Chatterjee; Ming-Tang Chen; Paul M. Chesler; Ilje Cho; Pierre Christian; John Conway; T. M. Crawford; Geoffrey B. Crew; Alejandro Cruz-Osorio; Jordy Davelaar; Mariafelicia De Laurentis; Roger Deane; Jessica Dempsey; Gregory Desvignes; Jason Dexter; Sheperd S. Doeleman; Heino Falcke; Joseph R. Farah; Vincent L. Fish; Ed Fomalont; Raquel Fraga-Encinas; Antonio Fuentes; Peter Galison; Charles F. Gammie; Boris Georgiev; Roman Gold; Arturo I. Gómez-Ruiz; Minfeng Gu; Mark Gurwell; Ronald Hesper; Luis C. Ho; Paul T. P. Ho; Mareki Honma; Chih-Wei Locutus Huang; Shiro Ikeda; Sara Issaoun; David J. James; Buell T. Jannuzi; Michael Janssen; Britton Jeter; Wu Jiang; Michael D. Johnson; Taehyun Jung; Mansour Karami; Ramesh Karuppusamy; Mark Kettenis; Dong-Jin Kim; Jongsoo Kim; Junhan Kim; Jun Yi Koay; Patrick M. Koch; Shoko Koyama; Michael Kramer; Carsten Kramer; Tod R. Lauer; Aviad Levis; Yan-Rong Li; Zhiyuan Li; Michael Lindqvist; Rocco Lico; Greg Lindahl; Jun Liu; Kuo Liu; Elisabetta Liuzzo; Wen Ping Lo; Andrei Lobanov; Laurent Loinard; Colin J. Lonsdale; Nicholas R. MacDonald; Jirong Mao; Nicola Marchili; Daniel P. Marrone; Alan P. Marscher; Satoki Matsushita; Lynn D. Matthews; Lia Medeiros; Karl M. Menten; Izumi Mizuno; Yosuke Mizuno; James M. Moran; Kotaro Moriyama; Monika Moscibrodzka; Cornelia Müller; Gibwa Musoke; Alejandro Mus Mejías; Hiroshi Nagai; Neil M. Nagar; Masanori Nakamura; Ramesh Narayan; Gopal Narayanan; Iniyan Natarajan; Chunchong Ni; Aristeidis Noutsos; Hector Olivares; Gisela N. Ortiz-León; Feryal Özel; Daniel C. M. Palumbo; Ue-Li Pen; Dominic W. Pesce; Vincent Piétu; Richard Plambeck; Aleksandar Popstefanija; Oliver Porth; Felix M. Pötzl; Ben Prather; Jorge A. Preciado-López; Hung Yi Pu; Ramprasad Rao; Alexander W. Raymond; Luciano Rezzolla; Angelo Ricarte; Bart Ripperda; Freek Roelofs; Eduardo Ros; Mel Rose; Alan L. Roy; Chet Ruszczyk; Kazi L.J. Rygl; David Sánchez-Arguelles; Tuomas Savolainen; F. Peter Schloerb; Lijing Shao; Des Small; Bong Won Sohn; Jason SooHoo; He Sun; Fumie Tazaki; Alexandra J. Tetarenko; Paul Tiede; Remo P. J. Tilanus; Michael Titus; Kenji Toma; Pablo Torne; Tyler Trent; Efthalia Traianou; Sascha Trippe; Ilse van Bemmel; Huib Jan van Langevelde; Daniel R. van Rossum; Jan Wagner; Derek Ward-Thompson; Jonathan Weintroub; Norbert Wex; Robert Wharton; Maciek Wielgus; George N. Wong; Qingwen Wu; Doosoo Yoon; André Young; Ken Young; Ziri Younsi; Feng Yuan; Guang Yao Zhao; Shan Shan Zhao; M. Orienti; R. Adam; E. O. Angüner; C. Arcaro; C. Armand; Halim Ashkar; Michael Backes; V. Baghmanyan; V. Barbosa Martins; Monica Barnard; D. Berge; Konrad Bernlöhr; M. de Bony de Lavergne; Mischa Breuhaus; Tomasz Bulik; S. Caroff; A. Carosi; T. Chand; J. Devin; A. Djannati-Ataï; Axel Donath; Victor Doroshenko; Christopher J. Duffy; Sabrina Einecke; G. Fichet de Clairfontaine; Gilles Fontaine; Stefano Gabici; J. F. Glicenstein; Maria Haupt; G. Hermann; Jim Hinton; Clemens Hoischen; Tim Holch; Dieter Horns; Marek Jamrozy; Felix Jankowsky; V. Joshi; I. Jung-Richardt; U. Katz; Bruno Khelifi; Stefan Klepser; Nu. Komin; R. Konno; K. Kosack; Dmitriy Kostunin; Iryna Lypova; Jonathan Mackey; D. Malyshev; Paolo Marchegiani; A. Marcowith; G. Martí-Devesa; Manuel Meyer; Rafal Moderski; M. Mohamed; L. Mohrmann; E. Moulin; A. Nayerhoda; F. Niederwanger; Jacek Niemiec; L. Oakes; Stefan Ohm; R. D. Parsons; G. Peron; Q. Piel; A. Priyana Noel; Michael Punch; P. Reichherzer; A. Reimer; Olaf Reimer; L. Rinchiuso; E. Ruiz-Velasco; V. Sahakian; S. Sailer; Andrea Santangelo; M. Scalici; H. M. Schutte; M. Seglar-Arroyo; A. Sinha; Andreas Specovius; Christian Stegmann; T. Tavernier; Regis Terrier; Michelle Tsirou; C. van Eldik; B. van Soelen; Johannes Veh; Christo Venter; Heinrich J. Völk; Zorawar Wadiasingh; R. J. White; Yu Wun Wong; A. Yusafzai; M. Zacharias; Davit Zargaryan; A. A. Zdziarski; A. Zech; Sylvia Zhu; J. Zorn; Samuel Zouari; V. A. Acciari; L. A. Antonelli; A. Arbet Engels; Ana Babić; Andrés Baquero; J. A. Barrio; J. Becerra González; Wlodek Bednarek; Elisa Bernardini; A. Berti; Ciro Bigongiari; Oscar Blanch; Giacomo Bonnoli; Bošnjak; G. Busetto; Giovanni Ceribella; Matteo Cerruti; Ashot Chilingarian; Stefan Cikota; Sidika Merve Colak; E. Colombo; Jose Luis Contreras; Juan Cortina; Giacomo D'Amico; P. Da Vela; Francesco Dazzi; A. De Angelis; B. De Lotto; Jose Miguel Delgado; C. Delgado Mendez; D. Depaoli; F. Di Pierro; L. Di Venere; E. Do Souto Espiñeira; D. Dominis Prester; Alice Donini; Daniela Dorner; Michele Doro; Dominik Elsaesser; V. Fallah Ramazani; Alicia Fattorini; Giovanna Ferrara; M. V. Fonseca; Lluis Font; Satoshi Fukami; R. J. García López; M. Garczarczyk; M. Gaug; Nicola Giglietto; F. Giordano; Pawel Gliwny; Nikola Godinovic; Jarred Gershon Green; D. Hadasch; Alexander Hahn; Lea Heckmann; J. Herrera; John Hoang; Toshiaki Inada; Sanae Inoue; Kazuma Ishio; I. Jiménez; Jenni Jormanainen; M. Karjalainen; Daniel Kerszberg; J. Kushida; Damir Lelas; F. Leone; Elina Lindfors; Saverio Lombardi; Francesco Longo; R. López-Coto; Marcos López-Moya; A. López-Oramas; S. Loporchio; B. Machado de Oliveira Fraga; Camilla Maggio; Manuela Mallamaci; G. Maneva; Mosè Mariotti; Stefano Menchiari; Simone Mender; S. Mićanović; D. Miceli; R. Mirzoyan; E. Molina; Abelardo Moralejo; Daniel Morcuende; Victoria Moreno; E. Moretti; Cosimo Nigro; Koji Noda; S. Nozaki; Y. Ohtani; Tomohiko Oka; J. Otero-Santos; S. Paiano; M. Palatiello; J. M. Paredes; C. Perennes; Massimo Persic; P. G. Prada Moroni; Elisa Prandini; Chaitanya Priyadarshi; Ivica Puljak; Wolfgang Rhode; Marc Ribó; J. Rico; Chiara Righi; A. Rugliancich; Narek Sahakyan; Tomoki Saito; Francesco Gabriele Saturni; Kasper B. Schmidt; Julian Sitarek; I. Snidaric; Dorota Sobczyńska; Alessia Spolon; A. Stamerra; Y. Suda; P. Temnikov; Luca Tosti; Santiago Ubach; J. van Scherpenberg; M. Vazquez Acosta; S. Ventura; Vassil Verguilov; V. Vitale; I. Vovk; D. Zarić; Wystan Benbow; A. Brill; M. Capasso; M. K. Daniel; Manel Errando; Q. Feng; Lucy Fortson; Tarek M. Hassan; W. Jin; P. Kaaret; Gernot Maier; Reshmi Mukherjee; Daniel Nieto; S. Patel; M. Pohl; E. Pueschel; K. Ragan; Marcos Santander; Tomoya Hirota; Lang Cui; Kotaro Niinuma; Nobuyuki Sakai; Satoko Sawada-Satoh; Kiyoaki Wajima; Na Wang; Xiang Liu; Yoshinori Yonekura;doi: 10.3847/2041-8213/abef71 , 10.48550/arxiv.2104.06855 , 10.18452/26482 , 10.3204/pubdb-2021-02289
handle: https://repository.ubn.ru.nl/handle/2066/234240 , 11588/852706 , 2066/234240 , 1887/3273725 , 11370/ac0f3897-b9e9-4976-ae3e-b9bb0ff27cc2 , 10261/254872 , 11368/3029214 , 20.500.11769/528437 , 11589/254743 , 2318/1877411 , 11245.1/32dcb8b3-e7b9-4e76-b7e8-a1adeef9de28 , 21.11116/0000-0009-E122-2 , 21.11116/0000-0009-E124-0 , 11365/1147696
doi: 10.3847/2041-8213/abef71 , 10.48550/arxiv.2104.06855 , 10.18452/26482 , 10.3204/pubdb-2021-02289
handle: https://repository.ubn.ru.nl/handle/2066/234240 , 11588/852706 , 2066/234240 , 1887/3273725 , 11370/ac0f3897-b9e9-4976-ae3e-b9bb0ff27cc2 , 10261/254872 , 11368/3029214 , 20.500.11769/528437 , 11589/254743 , 2318/1877411 , 11245.1/32dcb8b3-e7b9-4e76-b7e8-a1adeef9de28 , 21.11116/0000-0009-E122-2 , 21.11116/0000-0009-E124-0 , 11365/1147696
Full list of authors: EHT MWL Science Working Group; Algaba, J. C.; Anczarski, J.; Asada, K.; Baloković, M.; Chandra, S.; Cui, Y. -Z.; Falcone, A. D.; Giroletti, M.; Goddi, C.; Hada, K.; Haggard, D.; Jorstad, S.; Kaur, A.; Kawashima, T.; Keating, G.; Kim, J. -Y.; Kino, M.; Komossa, S.; Kravchenko, E. V.; Krichbaum, T. P.; Lee, S. -S.; Lu, R. -S.; Lucchini, M.; Markoff, S.; Neilsen, J.; Nowak, M. A.; Park, J.; Principe, G.; Ramakrishnan, V.; Reynolds, M. T.; Sasada, M.; Savchenko, S. S.; Williamson, K. E.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Barrett, John; Bintley, Dan; Benson, Bradford A.; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; Chael, Andrew; Chan, Chi-Kwan; Chatterjee, Shami; Chatterjee, Koushik; Chen, Ming-Tang; Chen, Yongjun; Chesler, Paul M.; Cho, Ilje; Christian, Pierre; Conway, John E.; Cordes, James M.; Crawford, Thomas M.; Crew, Geoffrey B.; Cruz-Osorio, Alejandro; Davelaar, Jordy; de Laurentis, Mariafelicia; Deane, Roger; Dempsey, Jessica; Desvignes, Gregory; Dexter, Jason; Doeleman, Sheperd S.; Eatough, Ralph P.; Falcke, Heino; Farah, Joseph; Fish, Vincent L.; Fomalont, Ed; Ford, H. Alyson; Fraga-Encinas, Raquel; Friberg, Per; Fromm, Christian M.; Fuentes, Antonio; Galison, Peter; Gammie, Charles F.; García, Roberto; Gentaz, Olivier; Georgiev, Boris; Gold, Roman; Gómez, José L.; Gómez-Ruiz, Arturo I.; Gu, Minfeng; Gurwell, Mark; Hecht, Michael H.; Hesper, Ronald; Ho, Luis C.; Ho, Paul; Honma, Mareki; Huang, Chih-Wei L.; Huang, Lei; Hughes, David H.; Ikeda, Shiro; Inoue, Makoto; Issaoun, Sara; James, David J.; Jannuzi, Buell T.; Janssen, Michael; Jeter, Britton; Jiang, Wu; Jiménez-Rosales, Alejandra; Johnson, Michael D.; Jung, Taehyun; Karami, Mansour; Karuppusamy, Ramesh; Kettenis, Mark; Kim, Dong-Jin; Kim, Jongsoo; Kim, Junhan; Koay, Jun Yi; Kofuji, Yutaro; Koch, Patrick M.; Koyama, Shoko; Kramer, Michael; Kramer, Carsten; Kuo, Cheng-Yu; Lauer, Tod R.; Levis, Aviad; Li, Yan-Rong; Li, Zhiyuan; Lindqvist, Michael; Lico, Rocco; Lindahl, Greg; Liu, Jun; Liu, Kuo; Liuzzo, Elisabetta; Lo, Wen-Ping; Lobanov, Andrei P.; Loinard, Laurent; Lonsdale, Colin; MacDonald, Nicholas R.; Mao, Jirong; Marchili, Nicola; Marrone, Daniel P.; Marscher, Alan P.; Martí-Vidal, Iván; Matsushita, Satoki; Matthews, Lynn D.; Medeiros, Lia; Menten, Karl M.; Mizuno, Izumi; Mizuno, Yosuke; Moran, James M.; Moriyama, Kotaro; Moscibrodzka, Monika; Müller, Cornelia; Musoke, Gibwa; Mejías, Alejandro Mus; Nagai, Hiroshi; Nagar, Neil M.; Nakamura, Masanori; Narayan, Ramesh; Narayanan, Gopal; Natarajan, Iniyan; Nathanail, Antonios; Neri, Roberto; Ni, Chunchong; Noutsos, Aristeidis; Okino, Hiroki; Olivares, Héctor; Ortiz-León, Gisela N.; Oyama, Tomoaki; Özel, Feryal; Palumbo, Daniel C. M.; Patel, Nimesh; Pen, Ue-Li; Pesce, Dominic W.; Piétu, Vincent; Plambeck, Richard; Popstefanija, Aleksandar; Porth, Oliver; Pötzl, Felix M.; Prather, Ben; Preciado-López, Jorge A.; Psaltis, Dimitrios; Pu, Hung-Yi; Rao, Ramprasad; Rawlings, Mark G.; Raymond, Alexander W.; Rezzolla, Luciano; Ricarte, Angelo; Ripperda, Bart; Roelofs, Freek; Rogers, Alan; Ros, Eduardo; Rose, Mel; Roshanineshat, Arash; Rottmann, Helge; Roy, Alan L.; Ruszczyk, Chet; Rygl, Kazi L. J.; Sánchez, Salvador; Sánchez-Arguelles, David; Savolainen, Tuomas; Schloerb, F. Peter; Schuster, Karl-Friedrich; Shao, Lijing; Shen, Zhiqiang; Small, Des; Sohn, Bong Won; Soohoo, Jason; Sun, He; Tazaki, Fumie; Tetarenko, Alexandra J.; Tiede, Paul; Tilanus, Remo P. J.; Titus, Michael; Toma, Kenji; Torne, Pablo; Trent, Tyler; Traianou, Efthalia; Trippe, Sascha; van Bemmel, Ilse; van Langevelde, Huib Jan; van Rossum, Daniel R.; Wagner, Jan; Ward-Thompson, Derek; Wardle, John; Weintroub, Jonathan; Wex, Norbert; Wharton, Robert; Wielgus, Maciek; Wong, George N.; Wu, Qingwen; Yoon, Doosoo; Young, André; Young, Ken; Younsi, Ziri; Yuan, Feng; Yuan, Ye-Fei; Zensus, J. Anton; Zhao, Guang-Yao; Zhao, Shan-Shan; Fermi Large Area Telescope Collaboration; Principe, G.; Giroletti, M.; D'Ammando, F.; Orienti, M.; H. E. S. S. Collaboration; Abdalla, H.; Adam, R.; Aharonian, F.; Benkhali, F. Ait; Angüner, E. O.; Arcaro, C.; Armand, C.; Armstrong, T.; Ashkar, H.; Backes, M.; Baghmanyan, V.; Barbosa Martins, V.; Barnacka, A.; Barnard, M.; Becherini, Y.; Berge, D.; Bernlöhr, K.; Bi, B.; Böttcher, M.; Boisson, C.; Bolmont, J.; de Lavergne, M. De Bony; Breuhaus, M.; Brun, F.; Brun, P.; Bryan, M.; Büchele, M.; Bulik, T.; Bylund, T.; Caroff, S.; Carosi, A.; Casanova, S.; Chand, T.; Chen, A.; Cotter, G.; Curyło, M.; Damascene Mbarubucyeye, J.; Davids, I. D.; Davies, J.; Deil, C.; Devin, J.; Dewilt, P.; Dirson, L.; Djannati-Ataï, A.; Dmytriiev, A.; Donath, A.; Doroshenko, V.; Duffy, C.; Dyks, J.; Egberts, K.; Eichhorn, F.; Einecke, S.; Emery, G.; Ernenwein, J. -P.; Feijen, K.; Fegan, S.; Fiasson, A.; de Clairfontaine, G. Fichet; Fontaine, G.; Funk, S.; Füßling, M.; Gabici, S.; Gallant, Y. A.; Giavitto, G.; Giunti, L.; Glawion, D.; Glicenstein, J. F.; Gottschall, D.; Grondin, M. -H.; Hahn, J.; Haupt, M.; Hermann, G.; Hinton, J. A.; Hofmann, W.; Hoischen, C.; Holch, T. L.; Holler, M.; Hörbe, M.; Horns, D.; Huber, D.; Jamrozy, M.; Jankowsky, D.; Jankowsky, F.; Jardin-Blicq, A.; Joshi, V.; Jung-Richardt, I.; Kasai, E.; Kastendieck, M. A.; Katarzyński, K.; Katz, U.; Khangulyan, D.; Khélifi, B.; Klepser, S.; Kluźniak, W.; Komin, Nu.; Konno, R.; Kosack, K.; Kostunin, D.; Kreter, M.; Lamanna, G.; Lemière, A.; Lemoine-Goumard, M.; Lenain, J. -P.; Levy, C.; Lohse, T.; Lypova, I.; Mackey, J.; Majumdar, J.; Malyshev, D.; Malyshev, D.; Marandon, V.; Marchegiani, P.; Marcowith, A.; Mares, A.; Martí-Devesa, G.; Marx, R.; Maurin, G.; Meintjes, P. J.; Meyer, M.; Moderski, R.; Mohamed, M.; Mohrmann, L.; Montanari, A.; Moore, C.; Morris, P.; Moulin, E.; Muller, J.; Murach, T.; Nakashima, K.; Nayerhoda, A.; de Naurois, M.; Ndiyavala, H.; Niederwanger, F.; Niemiec, J.; Oakes, L.; O'Brien, P.; Odaka, H.; Ohm, S.; Olivera-Nieto, L.; de Ona Wilhelmi, E.; Ostrowski, M.; Panter, M.; Panny, S.; Parsons, R. D.; Peron, G.; Peyaud, B.; Piel, Q.; Pita, S.; Poireau, V.; Noel, A. Priyana; Prokhorov, D. A.; Prokoph, H.; Pühlhofer, G.; Punch, M.; Quirrenbach, A.; Rauth, R.; Reichherzer, P.; Reimer, A.; Reimer, O.; Remy, Q.; Renaud, M.; Rieger, F.; Rinchiuso, L.; Romoli, C.; Rowell, G.; Rudak, B.; Ruiz-Velasco, E.; Sahakian, V.; Sailer, S.; Sanchez, D. A.; Santangelo, A.; Sasaki, M.; Scalici, M.; Schutte, H. M.; Schwanke, U.; Schwemmer, S.; Seglar-Arroyo, M.; Senniappan, M.; Seyffert, A. S.; Shafi, N.; Shiningayamwe, K.; Simoni, R.; Sinha, A.; Sol, H.; Specovius, A.; Spencer, S.; Spir-Jacob, M.; Stawarz, Ł.; Sun, L.; Steenkamp, R.; Stegmann, C.; Steinmassl, S.; Steppa, C.; Takahashi, T.; Tavernier, T.; Taylor, A. M.; Terrier, R.; Tiziani, D.; Tluczykont, M.; Tomankova, L.; Trichard, C.; Tsirou, M.; Tuffs, R.; Uchiyama, Y.; van der Walt, D. J.; van Eldik, C.; van Rensburg, C.; van Soelen, B.; Vasileiadis, G.; Veh, J.; Venter, C.; Vincent, P.; Vink, J.; Völk, H. J.; Vuillaume, T.; Wadiasingh, Z.; Wagner, S. J.; Watson, J.; Werner, F.; White, R.; Wierzcholska, A.; Wong, Yu Wun; Yusafzai, A.; Zacharias, M.; Zanin, R.; Zargaryan, D.; Zdziarski, A. A.; Zech, A.; Zhu, S. J.; Zorn, J.; Zouari, S.; Żywucka, N.; MAGIC Collaboration; Acciari, V. A.; Ansoldi, S.; Antonelli, L. A.; Engels, A. Arbet; Artero, M.; Asano, K.; Baack, D.; Babić, A.; Baquero, A.; de Almeida, U. Barres; Barrio, J. A.; Becerra González, J.; Bednarek, W.; Bellizzi, L.; Bernardini, E.; Bernardos, M.; Berti, A.; Besenrieder, J.; Bhattacharyya, W.; Bigongiari, C.; Biland, A.; Blanch, O.; Bonnoli, G.; Bošnjak, Ž.; Busetto, G.; Carosi, R.; Ceribella, G.; Cerruti, M.; Chai, Y.; Chilingarian, A.; Cikota, S.; Colak, S. M.; Colombo, E.; Contreras, J. L.; Cortina, J.; Covino, S.; D'Amico, G.; D'Elia, V.; da Vela, P.; Dazzi, F.; de Angelis, A.; de Lotto, B.; Delfino, M.; Delgado, J.; Delgado Mendez, C.; Depaoli, D.; di Pierro, F.; di Venere, L.; Do Souto Espiñeira, E.; Dominis Prester, D.; Donini, A.; Dorner, D.; Doro, M.; Elsaesser, D.; Ramazani, V. Fallah; Fattorini, A.; Ferrara, G.; Fonseca, M. V.; Font, L.; Fruck, C.; Fukami, S.; García López, R. J.; Garczarczyk, M.; Gasparyan, S.; Gaug, M.; Giglietto, N.; Giordano, F.; Gliwny, P.; Godinović, N.; Green, J. G.; Green, D.; Hadasch, D.; Hahn, A.; Heckmann, L.; Herrera, J.; Hoang, J.; Hrupec, D.; Hütten, M.; Inada, T.; Inoue, S.; Ishio, K.; Iwamura, Y.; Jiménez, I.; Jormanainen, J.; Jouvin, L.; Kajiwara, Y.; Karjalainen, M.; Kerszberg, D.; Kobayashi, Y.; Kubo, H.; Kushida, J.; Lamastra, A.; Lelas, D.; Leone, F.; Lindfors, E.; Lombardi, S.; Longo, F.; López-Coto, R.; López-Moya, M.; López-Oramas, A.; Loporchio, S.; Machado de Oliveira Fraga, B.; Maggio, C.; Majumdar, P.; Makariev, M.; Mallamaci, M.; Maneva, G.; Manganaro, M.; Mannheim, K.; Maraschi, L.; Mariotti, M.; Martínez, M.; Mazin, D.; Menchiari, S.; Mender, S.; Mićanović, S.; Miceli, D.; Miener, T.; Minev, M.; Miranda, J. M.; Mirzoyan, R.; Molina, E.; Moralejo, A.; Morcuende, D.; Moreno, V.; Moretti, E.; Neustroev, V.; Nigro, C.; Nilsson, K.; Nishijima, K.; Noda, K.; Nozaki, S.; Ohtani, Y.; Oka, T.; Otero-Santos, J.; Paiano, S.; Palatiello, M.; Paneque, D.; Paoletti, R.; Paredes, J. M.; Pavletić, L.; Peñil, P.; Perennes, C.; Persic, M.; Moroni, P. G. Prada; Prandini, E.; Priyadarshi, C.; Puljak, I.; Rhode, W.; Ribó, M.; Rico, J.; Righi, C.; Rugliancich, A.; Saha, L.; Sahakyan, N.; Saito, T.; Sakurai, S.; Satalecka, K.; Saturni, F. G.; Schleicher, B.; Schmidt, K.; Schweizer, T.; Sitarek, J.; Šnidarić, I.; Sobczynska, D.; Spolon, A.; Stamerra, A.; Strom, D.; Strzys, M.; Suda, Y.; Surić, T.; Takahashi, M.; Tavecchio, F.; Temnikov, P.; Terzić, T.; Teshima, M.; Tosti, L.; Truzzi, S.; Tutone, A.; Ubach, S.; van Scherpenberg, J.; Vanzo, G.; Vazquez Acosta, M.; Ventura, S.; Verguilov, V.; Vigorito, C. F.; Vitale, V.; Vovk, I.; Will, M.; Wunderlich, C.; Zarić, D.; VERITAS Collaboration; Adams, C. B.; Benbow, W.; Brill, A.; Capasso, M.; Christiansen, J. L.; Chromey, A. J.; Daniel, M. K.; Errando, M.; Farrell, K. A.; Feng, Q.; Finley, J. P.; Fortson, L.; Furniss, A.; Gent, A.; Giuri, C.; Hassan, T.; Hervet, O.; Holder, J.; Hughes, G.; Humensky, T. B.; Jin, W.; Kaaret, P.; Kertzman, M.; Kieda, D.; Kumar, S.; Lang, M. J.; Lundy, M.; Maier, G.; Moriarty, P.; Mukherjee, R.; Nieto, D.; Nievas-Rosillo, M.; O'Brien, S.; Ong, R. A.; Otte, A. N.; Patel, S.; Pfrang, K.; Pohl, M.; Prado, R. R.; Pueschel, E.; Quinn, J.; Ragan, K.; Reynolds, P. T.; Ribeiro, D.; Richards, G. T.; Roache, E.; Rulten, C.; Ryan, J. L.; Santander, M.; Sembroski, G. H.; Shang, R.; Weinstein, A.; Williams, D. A.; Williamson, T. J.; Eavn Collaboration; Hirota, Tomoya; Cui, Lang; Niinuma, Kotaro; Ro, Hyunwook; Sakai, Nobuyuki; Sawada-Satoh, Satoko; Wajima, Kiyoaki; Wang, Na; Liu, Xiang; Yonekura, Yoshinori The financial support of the German BMBF, MPG and HGF; the Italian INFN and INAF; the Swiss National Fund SNF; the ERDF under the Spanish Ministerio de Ciencia e Innovacion (MICINN) (FPA2017-87859-P, FPA2017-85668-P, FPA2017- 82729-C6-5-R, FPA2017-90566-REDC, PID2019-104114RBC31, PID2019-104114RB-C32, PID2019-105510GB-C31,PID 2019-107847RB-C41, PID2019-107847RB-C42, PID2019- 107988GB-C22); the Indian Department of Atomic Energy; the Japanese ICRR, the University of Tokyo, JSPS, and MEXT; the Bulgarian Ministry of Education and Science, National RI Roadmap Project DO1-268/16.12.2019 and the Academy of Finland grant No. 320045 is gratefully acknowledged. This work was also supported by the Spanish Centro de Excelencia “Severo Ochoa” SEV-2016-0588 and CEX2019- 000920-S, and “Maria de Maeztu” CEX2019-000918-M, the Unidad de Excelencia “Maria de Maeztu” MDM-2015-0509- 18-2 and the “la Caixa” Foundation (fellowship LCF/BQ/ PI18/11630012) and by the CERCA program of the Generalitat de Catalunya; by the Croatian Science Foundation (HrZZ) Project IP-2016-06-9782 and the University of Rijeka Project 13.12.1.3.02; by the DFG Collaborative Research Centers SFB823/C4 and SFB876/C3; the Polish National Research Centre grant UMO-2016/22/M/ST9/00382; and by the Brazilian MCTIC, CNPq, and FAPERJ. This research is supported by grants from the U.S. Department of Energy Office of Science, the U.S. National Science Foundation and the Smithsonian Institution, by NSERC in Canada, and by the Helmholtz Association in Germany. This research used resources provided by the Open Science Grid, which is supported by the National Science Foundation and the U.S. Department of Energy’s Office of Science, and resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231. We acknowledge the excellent work of the technical support staff at the Fred Lawrence Whipple Observatory and at the collaborating institutions in the construction and operation of the instrument. In 2017, the Event Horizon Telescope (EHT) Collaboration succeeded in capturing the first direct image of the center of the M87 galaxy. The asymmetric ring morphology and size are consistent with theoretical expectations for a weakly accreting supermassive black hole of mass ∼6.5 × 109 M o˙. The EHTC also partnered with several international facilities in space and on the ground, to arrange an extensive, quasi-simultaneous multi-wavelength campaign. This Letter presents the results and analysis of this campaign, as well as the multi-wavelength data as a legacy data repository. We captured M87 in a historically low state, and the core flux dominates over HST-1 at high energies, making it possible to combine core flux constraints with the more spatially precise very long baseline interferometry data. We present the most complete simultaneous multi-wavelength spectrum of the active nucleus to date, and discuss the complexity and caveats of combining data from different spatial scales into one broadband spectrum. We apply two heuristic, isotropic leptonic single-zone models to provide insight into the basic source properties, but conclude that a structured jet is necessary to explain M87's spectrum. We can exclude that the simultaneous γ-ray emission is produced via inverse Compton emission in the same region producing the EHT mm-band emission, and further conclude that the γ-rays can only be produced in the inner jets (inward of HST-1) if there are strongly particle-dominated regions. Direct synchrotron emission from accelerated protons and secondaries cannot yet be excluded. Peer reviewed
NARCIS arrow_drop_down NARCIS; The Astrophysical Journal LettersArticle . 2021IRIS - Università degli Studi di Catania; METIS Research Information System; NARCIS; Archivio Istituzionale della Ricerca - Politecnico di Bari; Archivio Istituzionale; The Astrophysical Journal Letters; Archivio della ricerca - Università degli studi di Napoli Federico II; Croatian Scientific Bibliography - CROSBIOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYData sources: European Union Open Data Portal; Sygma; IRIS - Università degli Studi di Catania; Crossref; METIS Research Information System; NARCIS; Archivio Istituzionale della Ricerca - Politecnico di Bari; Archivio Istituzionale; Archivio della ricerca - Università degli studi di Napoli Federico II; Croatian Scientific Bibliography - CROSBICORE (RIOXX-UK Aggregator)Article . 2021License: CC BYFull-Text: https://clok.uclan.ac.uk/37450/1/pdf.pdfData sources: CORE (RIOXX-UK Aggregator)University of Southern Denmark Research OutputArticle . 2021Data sources: University of Southern Denmark Research OutputThe Astrophysical Journal LettersArticle . 2021Data sources: University of Southern Denmark Research Outputedoc-Server. Open-Access-Publikationsserver der Humboldt-Universität zu BerlinArticle . 2021 . Peer-reviewedUniversity of Oulu Repository - JultikaArticle . 2021Data sources: University of Oulu Repository - JultikaOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2021Data sources: OA@INAF - Istituto Nazionale di AstrofisicaIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedAaltodoc Publication ArchiveArticle . 2021 . Peer-reviewedData sources: Aaltodoc Publication ArchiveLeiden University Scholarly Publications RepositoryOther literature type . 2021License: CC BYData sources: Leiden University Scholarly Publications RepositoryArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Archivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di Pisaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 54 citations 54 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!visibility 158visibility views 158 download downloads 335 Powered bymore_vert NARCIS arrow_drop_down NARCIS; The Astrophysical Journal LettersArticle . 2021IRIS - Università degli Studi di Catania; METIS Research Information System; NARCIS; Archivio Istituzionale della Ricerca - Politecnico di Bari; Archivio Istituzionale; The Astrophysical Journal Letters; Archivio della ricerca - Università degli studi di Napoli Federico II; Croatian Scientific Bibliography - CROSBIOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYData sources: European Union Open Data Portal; Sygma; IRIS - Università degli Studi di Catania; Crossref; METIS Research Information System; NARCIS; Archivio Istituzionale della Ricerca - Politecnico di Bari; Archivio Istituzionale; Archivio della ricerca - Università degli studi di Napoli Federico II; Croatian Scientific Bibliography - CROSBICORE (RIOXX-UK Aggregator)Article . 2021License: CC BYFull-Text: https://clok.uclan.ac.uk/37450/1/pdf.pdfData sources: CORE (RIOXX-UK Aggregator)University of Southern Denmark Research OutputArticle . 2021Data sources: University of Southern Denmark Research OutputThe Astrophysical Journal LettersArticle . 2021Data sources: University of Southern Denmark Research Outputedoc-Server. Open-Access-Publikationsserver der Humboldt-Universität zu BerlinArticle . 2021 . Peer-reviewedUniversity of Oulu Repository - JultikaArticle . 2021Data sources: University of Oulu Repository - JultikaOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2021Data sources: OA@INAF - Istituto Nazionale di AstrofisicaIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedAaltodoc Publication ArchiveArticle . 2021 . Peer-reviewedData sources: Aaltodoc Publication ArchiveLeiden University Scholarly Publications RepositoryOther literature type . 2021License: CC BYData sources: Leiden University Scholarly Publications RepositoryArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Archivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di Pisaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2021 Italy, FrancePublisher:Elsevier BV Publicly fundedFunded by:NSF | WoU-MMA:Astrophysics with..., NSF | Collaborative Research: M..., NSF | TeV Astrophysics with the... +9 projectsNSF| WoU-MMA:Astrophysics with a New Very-High-Energy Gamma-Ray Telescope ,NSF| Collaborative Research: MRI Consortium: Development of a Novel Telescope for Very High-Energy Gamma-Ray Astrophysics ,NSF| TeV Astrophysics with the VERITAS Gamma Ray Observatory ,NSF| Collaborative Research: MRI Consortium: Development of a Novel Telescope for Very High-Energy Gamma-Ray Astrophysics ,NSF| Particle and Gamma-Ray Astrophysics with HAWC/VERITAS (Utah Group Grant) ,NSF| Wou-MMA: Particle Astrophysics with VERITAS and CTA ,NSF| WoU-MMA: Operations of VERITAS in the Epoch 2019 to 2022 ,NSF| Gamma-Ray Astronomy and Cosmic-ray Astrophysics with the VERITAS and HAWC Observatories (University of Utah Group) ,NSF| Collaborative Research: MRI Consortium: Development of a Novel Telescope for Very High-Energy Gamma-Ray Astrophysics ,NSF| Astrophysics with Very-High-Energy Gamma Rays ,NSF| Multi-Messenger Astrophysics with the Cherenkov Telescope Array ,NSF| Astroparticle Physics with the VERITAS and CTA Gamma-Ray ObservatoriesC. B. Adams; Ruben Alfaro; G. Ambrosi; M. Ambrosio; Carla Aramo; T. C. Arlen; P. I. Batista; Wystan Benbow; B. Bertucci; Elisabetta Bissaldi; Jonathan Biteau; M. Bitossi; A. Boiano; C. Bonavolontà; Richard Bose; A. Bouvier; A. Brill; A. M. Brown; J. H. Buckley; Karen Byrum; R. A. Cameron; Rodolfo Canestrari; M. Capasso; M. Caprai; Corbin Covault; D. Depaoli; Manel Errando; S. J. Fegan; Q. Feng; E. Fiandrini; G. M. Foote; P. Fortin; Stefan Funk; Amy Furniss; Fernando Garfias; Alasdair E. Gent; Nicola Giglietto; Francesco Giordano; Enrico Giro; Maria Magdalena González; V. J. Guarino; R. Halliday; Olivier Hervet; Jamie Holder; G. Hughes; T. B. Humensky; Maria Ionica; Arturo Iriarte; W. Jin; C. A. Johnson; P. Kaaret; David Kieda; B. Kim; A. Kuznetsov; Jonathan S. Lapington; F. Licciulli; S. Loporchio; V. Masone; K. Meagher; Thomas Meures; B. A. W. Mode; S. I. Mognet; Reshmi Mukherjee; T. Nguyen; Daniel Nieto; Akira Okumura; N. Otte; N. La Palombara; F. R. Pantaleo; Riccardo Paoletti; G. Pareschi; A. Petrashyk; F. Di Pierro; E. Pueschel; P. T. Reynolds; D. Ribeiro; Gordon T. Richards; E. Roache; D. Ross; Julien Rousselle; Andrea Rugliancich; J. Ruíz-Díaz-Soto; Marcos Santander; S. Schlenstedt; Michael Schneider; Salvo Scuderi; R. Shang; G. Sironi; B. Stevenson; L. Stiaccini; Hiroyasu Tajima; L. P. Taylor; J. Thornhill; L. Tosti; Gagik Tovmassian; V. Vagelli; M. Valentino; Justin Vandenbroucke; Vladimir Vassiliev; L. Di Venere; S. P. Wakely; Jason John Watson; R. J. White; P. Wilcox; David A. Williams; Matthew Wood; P. Yu; A. Zink;The Schwarzschild-Couder Telescope (SCT) is a telescope concept proposed for the Cherenkov Telescope Array. It employs a dual-mirror optical design to remove comatic aberrations over an $8^{\circ}$ field of view, and a high-density silicon photomultiplier camera (with a pixel resolution of 4 arcmin) to record Cherenkov emission from cosmic ray and gamma-ray initiated particle cascades in the atmosphere. The prototype SCT (pSCT), comprising a 9.7 m diameter primary mirror and a partially instrumented camera with 1536 pixels, has been constructed at the Fred Lawrence Whipple Observatory. The telescope was inaugurated in January 2019, with commissioning continuing throughout 2019. We describe the first campaign of observations with the pSCT, conducted in January and February of 2020, and demonstrate the detection of gamma-ray emission from the Crab Nebula with a statistical significance of $8.6\sigma$. Comment: 13 pages, 12 figures, 3 tables, submitted to Astroparticle Physics
Archivio Istituziona... arrow_drop_down Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 15 citations 15 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!more_vert Archivio Istituziona... arrow_drop_down Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 France, IrelandPublisher:Cambridge University Press (CUP) Publicly fundedFunded by:SFI | Nonlinear wave-current in...SFI| Nonlinear wave-current interactions in the nearshore: addressing the role of vorticity and nonlinearity in the modelling of ocean energyAuthors: Didier Clamond; David Henry;Didier Clamond; David Henry;handle: 10468/12188
International audience; The aim of this note is to examine the efficacy of a recently developed approach to the recovery of nonlinear water waves from pressure measurements at the seabed, by applying it to the celebrated extreme Stokes wave.
Cork Open Research A... arrow_drop_down Cork Open Research Archive (CORA)Article . 2020License: CC BY NC NDData sources: Cork Open Research Archive (CORA)Journal of Fluid MechanicsArticle . 2020 . Peer-reviewedLicense: Cambridge Core User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Full-Text: https://hal.science/hal-02638111/documenthttps://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Cork Open Research A... arrow_drop_down Cork Open Research Archive (CORA)Article . 2020License: CC BY NC NDData sources: Cork Open Research Archive (CORA)Journal of Fluid MechanicsArticle . 2020 . Peer-reviewedLicense: Cambridge Core User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Full-Text: https://hal.science/hal-02638111/documenthttps://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1017/jfm.2020.729&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 United States, FrancePublisher:American Physical Society (APS) Publicly fundedFunded by:NSF | Gravitational Radiation a..., NSF | Maximizing Science Output..., UKRI | Friction Stir Welding Cra... +3 projectsNSF| Gravitational Radiation and Relativistic Astrophysics ,NSF| Maximizing Science Output of LIGO: Improved Detectors and Data Analysis ,UKRI| Friction Stir Welding Crawler for Internal Repair and Refurbishment of Pipelines - FSWBot ,EC| FunFiCO ,EC| BinGraSp ,UKRI| The Lancaster, Manchester, Sheffield Consortium for Fundamental Physics: Particle Physics from the LHC to the UniverseSarp Akcay; Sam R. Dolan; Chris Kavanagh; Jordan Moxon; Niels Warburton; Barry Wardell;We present the gravitational-wave flux balance law in an extreme mass-ratio binary with a spinning secondary. This law relates the flux of energy (angular momentum) radiated to null infinity and through the event horizon to the local change in the secondary's orbital energy (angular momentum) for generic (non-resonant) bound orbits in Kerr spacetime. As an explicit example we compute these quantities for a spin-aligned body moving on a circular orbit around a Schwarzschild black hole. We perform this calculation both analytically, via a high-order post-Newtonian expansion, and numerically in two different gauges. Using these results we demonstrate explicitly that our new balance law holds. Comment: Minor typos corrected
Caltech Authors arrow_drop_down https://doi.org/10.1103/physre...Article . 2020 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . Preprint . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.102.064013&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 4visibility views 4 download downloads 19 Powered bymore_vert Caltech Authors arrow_drop_down https://doi.org/10.1103/physre...Article . 2020 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . Preprint . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.102.064013&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Other literature type , Preprint , Article 2020 France, Spain, Spain, FinlandPublisher:Copernicus GmbH Publicly fundedFunded by:UKRI | IFS-NET: Insect Food Secu..., EC | ACTRIS-2UKRI| IFS-NET: Insect Food Security NETwork ,EC| ACTRIS-2A. Cuesta-Mosquera; G. Močnik; G. Močnik; G. Močnik; L. Drinovec; L. Drinovec; L. Drinovec; T. Müller; S. Pfeifer; M. C. Minguillón; B. Briel; P. Buckley; V. Dudoitis; J. Fernández-García; M. Fernández-Amado; J. Ferreira De Brito; V. Riffault; H. Flentje; E. Heffernan; N. Kalivitis; A.-C. Kalogridis; H. Keernik; H. Keernik; L. Marmureanu; K. Luoma; A. Marinoni; M. Pikridas; G. Schauer; N. Serfozo; H. Servomaa; G. Titos; J. Yus-Díez; J. Yus-Díez; N. Zioła; A. Wiedensohler;handle: 10261/242385 , 2183/28139
Aerosolized black carbon is monitored worldwide to quantify its impact on air quality and climate. Given its importance, measurements of black carbon mass concentrations must be conducted with instruments operating in quality-checked and ensured conditions to generate data which are reliable and comparable temporally and geographically. In this study, we report the results from the largest characterization and intercomparison of filter-based absorption photometers, the Aethalometer model AE33, belonging to several European monitoring networks. Under controlled laboratory conditions, a total of 23 instruments measured mass concentrations of black carbon from three well-characterized aerosol sources: synthetic soot, nigrosin particles, and ambient air from the urban background of Leipzig, Germany. The objective was to investigate the individual performance of the instruments and their comparability; we analyzed the response of the instruments to the different aerosol sources and the impact caused by the use of obsolete filter materials and the application of maintenance activities. Differences in the instrument-to-instrument variabilities from equivalent black carbon (eBC) concentrations reported at 880 nm were determined before maintenance activities (for soot measurements, average deviation from total least square regression was −2.0 % and the range −16 % to 7 %; for nigrosin measurements, average deviation was 0.4 % and the range −15 % to 17 %), and after they were carried out (for soot measurements, average deviation was −1.0 % and the range −14 % to 8 %; for nigrosin measurements, the average deviation was 0.5 % and the range −12 % to 15 %). The deviations are in most of the cases explained by the type of filter material employed by the instruments, the total particle load on the filter, and the flow calibration. The results of this intercomparison activity show that relatively small unit-to-unit variability of AE33-based particle light absorbing measurements is possible with well-maintained instruments. It is crucial to follow the guidelines for maintenance activities and the use of the proper filter tape in the AE33 to ensure high quality and comparable black carbon (BC) measurements among international observational networks. ACTRIS and COLOSSAL provided financial support for the execution of the experiments. Instrument S04-00387 is operated and maintained thanks to the Spanish Ministry of Science and Innovation (project nos. CGL2016-81092-R, CGL2017-42 90884REDT, and RTI2018.101154.A.I00). Gloria Titos is funded by the Juan de la Cierva-Incorporación postdoctoral program (grant no. IJCI-2016-29838). IMT Lille Douai (Joel Ferreira De Brito, Veronique Riffault) received financial support from the Labex CaPPA project, which is funded by the French National Research Agency (ANR) through the PIA (Programme d'Investissement d'Avenir) (contract no. ANR-11-LABX-0005-01), and the CLIMIBIO project; both projects are financed by the Regional Council “Hauts-de-France” and the European Regional Development Fund (ERDF). The operation of instruments S00-00055 and S02-00156 is funded by the projects CRISOL (MINECO/AEI/FEDER, UE; grant no. CGL2017-85344-R) and TIGAS-CM (grant no. Y2018/EMT-5177). Peer reviewed
Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2021License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAAtmospheric Measurement Techniques (AMT)Other literature type . 2021Data sources: Copernicus Publicationshttps://doi.org/10.5194/amt-20...Preprint . 2020 . Peer-reviewedLicense: CC BYData sources: CrossrefRepositorio da Universidade da CoruñaArticle . 2021License: CC BYData sources: Repositorio da Universidade da CoruñaRecolector de Ciencia Abierta, RECOLECTA; Atmospheric Measurement TechniquesArticle . 2021 . Peer-reviewedLicense: CC BYHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiAtmospheric Measurement Techniques (AMT)Other literature type . 2020Data sources: Copernicus PublicationsRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/amt-2020-344&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 21 citations 21 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 25visibility views 25 download downloads 68 Powered bymore_vert Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2021License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAAtmospheric Measurement Techniques (AMT)Other literature type . 2021Data sources: Copernicus Publicationshttps://doi.org/10.5194/amt-20...Preprint . 2020 . Peer-reviewedLicense: CC BYData sources: CrossrefRepositorio da Universidade da CoruñaArticle . 2021License: CC BYData sources: Repositorio da Universidade da CoruñaRecolector de Ciencia Abierta, RECOLECTA; Atmospheric Measurement TechniquesArticle . 2021 . Peer-reviewedLicense: CC BYHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiAtmospheric Measurement Techniques (AMT)Other literature type . 2020Data sources: Copernicus PublicationsRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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description Publicationkeyboard_double_arrow_right Preprint , Article 2021 FrancePublisher:EDP Sciences Publicly fundedQuentin Kral; J. E. Pringle; A. Guilbert-Lepoutre; Luca Matrà; Julianne I. Moses; Emmanuel Lellouch; Mark C. Wyatt; N. Biver; Dominique Bockelée-Morvan; Amy Bonsor; F. Le Petit; G. Randall Gladstone;Gas has been detected in many exoplanetary systems ($>$10 Myr), thought to be released in the destruction of volatile-rich planetesimals orbiting in exo-Kuiper belts. In this letter, we aim to explore whether gas is also expected in the Kuiper belt (KB) in our Solar System. To quantify the gas release in our Solar System, we use models for gas release that have been applied to extrasolar planetary systems, as well as a physical model that accounts for gas released due to the progressive internal warming of large planetesimals. We find that only bodies larger than about 4 km can still contain CO ice after 4.6 Gyr of evolution. This finding may provide a clue as to why Jupiter-family comets, thought to originate in the Kuiper belt, are deficient in CO compared to Oort-clouds comets. We predict that gas is still produced in the KB right now at a rate of $2 \times 10^{-8}$ M$_\oplus$/Myr for CO and orders of magnitude more when the Sun was younger. Once released, the gas is quickly pushed out by the Solar wind. Therefore, we predict a gas wind in our Solar System starting at the KB location and extending far beyond with regards to the heliosphere with a current total CO mass of $\sim 2 \times 10^{-12}$ M$_\oplus$. We also predict the existence of a slightly more massive atomic gas wind made of carbon and oxygen (neutral and ionized) with a mass of $\sim 10^{-11}$ M$_\oplus$. We predict that gas is currently present in our Solar System beyond the Kuiper belt and that although it cannot be detected with current instrumentation, it could be observed in the future with an in situ mission using an instrument similar to Alice on New Horizons with larger detectors. Our model of gas release due to slow heating may also work for exoplanetary systems and provide the first real physical mechanism for the gas observations. accepted for publication as a Letter to the editor in A&A; abstract shortened; 15 pages, 5 figures, 4 tables
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/202141783&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 6 citations 6 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/202141783&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Conference object , Preprint 2021 Switzerland, France, France, Netherlands, Germany, France, PolandPublisher:Sissa Medialab Funded by:IRCIRCAlison Mitchell; Sami Caroff; Jim Hinton; L. Mohrmann; Felix Aharonian; Faical Ait-Benkhali; Oguzhan Anguener; C. Arcaro; Celine Armand; Tom Armstrong; Halim Ashkar; Michael Backes; Vardan Baghmanyan; Victor Barbosa Martins; Anna Barnacka; Monica Barnard; Rowan Batzofin; David Berge; K. Bernloehr; B. Bi; Markus Boettcher; Catherine Boisson; J. Bolmont; Mathieu Bony; Mischa Breuhaus; Robert Brose; Francois Brun; Tomasz Bulik; Floriane Cangemi; Sabrina Casanova; Jaqueline Catalano; Pauline Chambery; T. Chand; A. W. Chen; Garret Cotter; Malgorzata Curlo; Hannah Dalgleish; Jean Damascene Mbarubucyeye; Isak Delberth Davids; James Davies; Justine Devin; Arache Djannati-Ataï; Anton Dmytriiev; Axel Donath; Victor Doroshenko; Lente Dreyer; Kathrin Egberts; Sabrina Einecke; Jean-Pierre Ernenwein; S. J. Fegan; Kirsty Feijen; A. Fiasson; Lott Frans; Stefano Gabici; Yves Gallant; Gianluca Giavitto; L. Giunti; Dorit Glawion; J. F. Glicenstein; M.-H. Grondin; Sumari Hattingh; Maria Haupt; German Hermann; Werner Hofmann; Clemens Hoischen; Tim Holch; Markus Holler; Zhiqiu Huang; David Huber; M. Hörbe; Marek Jamrozy; Felix Jankowsky; Vikas Joshi; Ira Jung; E. Kasai; Krzysztof Katarzynski; U. Katz; Dmitry Khangulyan; Bruno Khelifi; Stefan Klepser; Wlodek Kluzniak; R. Konno; K. Kosack; Dmitriy Kostunin; Michael Kreter; Gašper Kukec Mezek; Anu Kundu; Sébastien Le Stum; M. Lemoine-Goumard; J.-P. Lenain; Fabian Leuschner; C. Levy; Thomas Lohse; Anna Luashvili; Iryna Lypova; Jonathan Mackey; Jhilik Majumdar; D. Malyshev; Vincent Marandon; Paolo Marchegiani; Guillem Marti'i-Devesa; Ramin Marx; Gilles Maurin; P. J. Meintjes; Manuel Meyer; Rafal Moderski; Alessandro Montanari; C. Moore; Paul Morris; Emmanuel Moulin; Jacques Muller; Thomas Murach; Mathieu Naurois; Amid Nayerhoda; Hambeleleni Ndiyavala; Jacek Niemiec; Angel Noel; P. T. O'Brien; Laenita Lorraine Oberholzer; Stefan Ohm; Laura Olivera-Nieto; Michal Ostrowski; Sebastian Panny; M. Panter; Dan Parsons; G. Peron; Santiago Pita; V. Poireau; D. A. Prokhorov; Heike Prokoph; Gerd Puehlhofer; Michael Punch; Andreas Quirrenbach; P. Reichherzer; Anita Reimer; Olaf Reimer; Q. Remy; Matthieu Renaud; Frank M. Rieger; Carlo Romoli; Gavin Rowell; B. Rudak; Edna Ruiz Velasco; V. Sahakian; S. Sailer; David Sanchez; Andrea Santangelo; Manami Sasaki; Johannes Schaefer; Hester Schutte; Ullrich Schwanke; Fabian Schüssler; Mohanraj Senniappan; Albert Seyffert; Jimmy N.S. Shapopi; Rachel Simoni; Atreyee Sinha; Helene Sol; Andreas Specovius; Samuel Timothy Spencer; Marion Spir-Jacob; Lukasz Stawarz; Riaan Steenkamp; Christian Stegmann; S. Steinmassl; Constantin Steppa; Lei Sun; Tadayuki Takahashi; Takaaki Tanaka; Thomas Tavernier; Andrew Taylor; Regis Terrier; Hannes Thiersen; Charles Thorpe-Morgan; Martin Tluczykont; Lenka Tomankova; Michelle Tsirou; Naomi Tsuji; R. J. Tuffs; Yasunobu Uchiyama; Johann van der Walt; Christopher van Eldik; Carlo van Rensburg; Brian van Soelen; G. Vasileiadis; Johannes Veh; Jacco Vink; Heinrich J. Völk; Stefan Wagner; Jason John Watson; Felix Werner; Richard White; Alicja Wierzcholska; Yu Wun Wong; A. Yusafzai; Roberta Zanin; Davit Zargaryan; A. A. Zdziarski; Andreas Zech; Sylvia Zhu; Andreas Zmija; N. Zywucka;Highly extended gamma-ray emission around the Geminga pulsar was discovered by Milagro and verified by HAWC. Despite many observations with Imaging Atmospheric Cherenkov Telescopes (IACTs), detection of gamma-ray emission on angular scales exceeding the IACT field-of-view has proven challenging. Recent developments in analysis techniques have enabled the detection of significant emission around Geminga in archival data with H.E.S.S.. In 2019, further data on the Geminga region were obtained with an adapted observation strategy. Following the announcement of the detection of significant TeV emission around Geminga in archival data, in this contribution we present the detection in an independent dataset. New analysis results will be presented, and emphasis given to the technical challenges involved in observations of highly extended gamma-ray emission with IACTs. Proceedings of 37th International Cosmic Ray Conference PoS: Proceedings of Science, 395 ISSN:1824-8039
MPG.PuRe arrow_drop_down Digitala Vetenskapliga Arkivet - Academic Archive On-lineArticle . 2023 . Peer-reviewedJagiellonian University RepositoryConference object . 2022Data sources: Jagiellonian University RepositoryHAL AMU; Mémoires en Sciences de l'Information et de la Communication; HAL-CEAArticle . 2023License: CC BYFull-Text: https://hal.science/hal-04080197/documentMémoires en Sciences de l'Information et de la CommunicationConference object . 2021add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.22323/1.395.0780&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 8 citations 8 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert MPG.PuRe arrow_drop_down Digitala Vetenskapliga Arkivet - Academic Archive On-lineArticle . 2023 . Peer-reviewedJagiellonian University RepositoryConference object . 2022Data sources: Jagiellonian University RepositoryHAL AMU; Mémoires en Sciences de l'Information et de la Communication; HAL-CEAArticle . 2023License: CC BYFull-Text: https://hal.science/hal-04080197/documentMémoires en Sciences de l'Information et de la CommunicationConference object . 2021add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.22323/1.395.0780&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2021 France, ItalyPublisher:Wiley Godard M.; Carter E. J.; Decrausaz T.; Lafay R.; Bennett E.; Kourim F.; Obeso J. ‐C.; Michibayashi K.; Harris M.; Coggon J. A.; Teagle D. A. H.; Kelemen P. B.; the Oman Drilling Project Phase 1 Science Party (include Laura Crispini); L. Crispini;handle: 11567/1067756
AbstractThe transition from the Semail ophiolite mantle to the underlying metamorphic sole was drilled at ICDP OmanDP Hole BT1B. We analyzed the bulk major, volatile and trace element compositions of the mantle‐derived listvenite series and metamorphic rocks, with the aim to constrain chemical transfers associated with peridotite carbonation along the ophiolite basal thrust. The listvenite series comprise variously carbonated serpentinites and (fuchsite‐bearing) listvenites. They have high CO2 (up to 43 wt.%) and variable H2O (0–12 wt.%). Yet, they have compositions close to that of the basal banded peridotites for most major and lithophile trace elements, with fuchsite‐bearing listvenites overlapping in composition with amphibole‐bearing basal lherzolites (e.g., Al2O3 = 0.1–2.2 wt.%; Yb = 0.05–1 x CI‐chondrite). The protolith of the listvenite series was likely similar in structure and composition to serpentinized banded peridotites which immediately overlie the metamorphic sole elsewhere in Oman. The listvenite series are enriched in fluid mobile elements (FME) compared to Semail peridotites (up to ∼103–104 x Primitive Mantle), with concentrations similar to the underthrusted metabasalts and/or metasediments for Cs, Sr and Ca and sometimes even higher for Pb, Li, As, and Sb (e.g., Li up to 130 μg/g; As up to 170 μg/g). We also observe a decoupling between Sr‐Ca enrichments and other FME, indicating interactions with several batches of deep CO2‐rich fluids transported along the basal thrust. These results suggest that peridotite carbonation could represent one of the major trap‐and‐release mechanisms for carbon, water and FME along convergent margins.
https://hal.archives... arrow_drop_down Journal of Geophysical Research Solid EarthArticle . 2021 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2021Full-Text: https://hal.science/hal-03501317/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/essoar.10507497.1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu4 citations 4 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert https://hal.archives... arrow_drop_down Journal of Geophysical Research Solid EarthArticle . 2021 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2021Full-Text: https://hal.science/hal-03501317/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/essoar.10507497.1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2021 FrancePublisher:Wiley Publicly fundedCorentin Louis; Ph. Zarka; K. Dabidin; P.-A. Lampson; F. P. Magalhães; A. Boudouma; M. S. Marques; Baptiste Cecconi;AbstractThe observations from the Juno spacecraft in polar orbit of Jupiter provide for the first time a complete view of Jupiter's radio emissions from all latitudes. Characterizing the latitudinal distribution of radio emissions' occurrence and intensity is a useful step for elucidating their origin. Here, we analyze for that purpose the first 3 years of observations from the Waves experiment on the Juno spacecraft (mid‐2016 to mid‐2019). Two prerequisites for the construction of the latitudinal distribution of intensities for each Jovian radio component are (a) to work with absolute flux densities and (b) to be able to associate each radio measurement with a specific radio component. Accordingly, we develop a method to convert the Juno/Waves data in flux densities and then we build a catalog of all Jovian radio components over the first 3 years of Juno's orbital mission. From these, we derive occurrence and intensity distributions versus observer's latitude and frequency for each component; these will be the basis for future detailed studies and interpretations of each component's characteristics and origin.
Journal of Geophysic... arrow_drop_down Journal of Geophysical Research Space PhysicsArticle . 2021 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2021Full-Text: https://hal.science/hal-03368294/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/essoar.10506795.1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 4 citations 4 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Journal of Geophysic... arrow_drop_down Journal of Geophysical Research Space PhysicsArticle . 2021 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2021Full-Text: https://hal.science/hal-03368294/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1002/essoar.10506795.1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2021 France, United Kingdom, FrancePublisher:Oxford University Press (OUP) Publicly fundedFunded by:IRC, EC | NewWorlds, EC | GPRV +2 projectsIRC ,EC| NewWorlds ,EC| GPRV ,EC| ASTROFLOW ,UKRI| Astronomy at St Andrews 2018-2021Robert D. Kavanagh; Aline A. Vidotto; Baptiste Klein; Moira Jardine; Jean-François Donati; Dúalta Ó Fionnagáin;handle: 10023/23042
There have recently been detections of radio emission from low-mass stars, some of which are indicative of star-planet interactions. Motivated by these exciting new results, in this paper we present Alfv\'en wave-driven stellar wind models of the two active planet-hosting M dwarfs Prox Cen and AU Mic. Our models incorporate large-scale photospheric magnetic field maps reconstructed using the Zeeman-Doppler Imaging method. We obtain a mass-loss rate of $0.25~\dot{M}_{\odot}$ for the wind of Prox Cen. For the young dwarf AU Mic, we explore two cases: a low and high mass-loss rate. Depending on the properties of the Alfv\'en waves which heat the corona in our wind models, we obtain mass-loss rates of $27$ and $590~\dot{M}_{\odot}$ for AU Mic. We use our stellar wind models to assess the generation of electron cyclotron maser instability emission in both systems, through a mechanism analogous to the sub-Alfv\'enic Jupiter-Io interaction. For Prox Cen we do not find any feasible scenario where the planet can induce radio emission in the star's corona, as the planet orbits too far from the star in the super-Alfv\'enic regime. However, in the case that AU Mic has a stellar wind mass-loss rate of $27~\dot{M}_{\odot}$, we find that both planets b and c in the system can induce radio emission from $\sim10$ MHz to 3 GHz in the corona of the host star for the majority of their orbits, with peak flux densities of $\sim10$ mJy. Detection of such radio emission would allow us to place an upper limit on the mass-loss rate of the star. Comment: 8 pages, 5 figures. Accepted for publication in MNRAS
Monthly Notices of t... arrow_drop_down Monthly Notices of the Royal Astronomical SocietyOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYSt Andrews Research RepositoryArticle . 2021 . Peer-reviewedData sources: St Andrews Research Repositoryhttps://doi.org/10.48550/arxiv...Article . 2021License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1093/mnras/stab929&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 35 citations 35 popularity Top 1% influence Average impulse Top 10% Powered by BIP!visibility 3visibility views 3 download downloads 13 Powered bymore_vert Monthly Notices of t... arrow_drop_down Monthly Notices of the Royal Astronomical SocietyOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYSt Andrews Research RepositoryArticle . 2021 . Peer-reviewedData sources: St Andrews Research Repositoryhttps://doi.org/10.48550/arxiv...Article . 2021License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1093/mnras/stab929&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint , Other literature type 2021 Germany, Denmark, Italy, Italy, Netherlands, Italy, Italy, Spain, Netherlands, Italy, Netherlands, Croatia, Italy, United States, Germany, France, Finland, Italy, Italy, Netherlands, Netherlands, Italy, Croatia, Netherlands, Poland, Netherlands, Italy, France, Bulgaria, France, FrancePublisher:American Astronomical Society Publicly fundedFunded by:EC | RadioNet, NSF | Collaborative Research: B..., AKA | Physics of Black Hole-Pow... +17 projectsEC| RadioNet ,NSF| Collaborative Research: Building an Event Horizon Telescope: (Sub)millimeter VLBI from the South Pole Telescope ,AKA| Physics of Black Hole-Powered Jets ,EC| PROBIST ,NSERC ,NSF| Graduate Research Fellowship Program (GRFP) ,NWO| From micro- to mega-scales: understanding how black holes shape the local Universe ,NSF| CyVerse: Cyberinfrastructure for the Life Sciences ,NSF| Physics Frontier Center at the Kavli Institute for Cosmological Physics: Pushing Cosmology to the Edge ,NSF| The Arizona Radio Observatory: Surveying the ISM through Millimeter and Sub-millimeter Spectroscopy ,NSF| The iPlant Collaborative: Cyberinfrastructure for the Life Sciences ,EC| BLACKHOLECAM ,AKA| Physics of Black Hole-Powered Jets ,NSF| PSCIC Full Proposal: The iPlant Collaborative: A Cyberinfrastructure-Centered Community for a New Plant Biology ,AKA| Physics of Black Hole-Powered Jets ,AKA| Intrinsic Very High Energy Gamma-ray Emission of Blazars ,NSF| Cosmological Research with the 10-meter South Pole Telescope ,HRZZ| Very high energy gamma-ray astronomy with the MAGIC and CTA telescopes ,AKA| From quasars to geodesy: how astronomy can enable a new era in ultra-precise geodetic measurements / Consortium: NT-VGOS ,NSF| Collaborative Research: Building an Event Horizon Telescope: (Sub)millimeter VLBI from the South Pole TelescopeJuan-Carlos Algaba; Jadyn Anczarski; Keiichi Asada; M. Balokovic; S. Chandra; Yuzhu Cui; A. D. Falcone; Marcello Giroletti; Ciriaco Goddi; Kazuhiro Hada; Daryl Haggard; Tomohisa Kawashima; Garrett K. Keating; Motoki Kino; S. Komossa; E. V. Kravchenko; Sera Markoff; J. Neilsen; Jongho Park; G. Principe; V. Ramakrishnan; Mahito Sasada; Kazunori Akiyama; Antxon Alberdi; Richard Anantua; Rebecca Azulay; Anne Kathrin Baczko; David Ball; Bradford Benson; Lindy Blackburn; Raymond Blundell; Katherine L. Bouman; Geoffrey C. Bower; Hope Boyce; Christiaan D. Brinkerink; Roger Brissenden; Silke Britzen; Avery E. Broderick; Dominique Broguiere; Thomas Bronzwaer; Do-Young Byun; Andrew Chael; Chi-kwan Chan; Shami Chatterjee; Koushik Chatterjee; Ming-Tang Chen; Paul M. Chesler; Ilje Cho; Pierre Christian; John Conway; T. M. Crawford; Geoffrey B. Crew; Alejandro Cruz-Osorio; Jordy Davelaar; Mariafelicia De Laurentis; Roger Deane; Jessica Dempsey; Gregory Desvignes; Jason Dexter; Sheperd S. Doeleman; Heino Falcke; Joseph R. Farah; Vincent L. Fish; Ed Fomalont; Raquel Fraga-Encinas; Antonio Fuentes; Peter Galison; Charles F. Gammie; Boris Georgiev; Roman Gold; Arturo I. Gómez-Ruiz; Minfeng Gu; Mark Gurwell; Ronald Hesper; Luis C. Ho; Paul T. P. Ho; Mareki Honma; Chih-Wei Locutus Huang; Shiro Ikeda; Sara Issaoun; David J. James; Buell T. Jannuzi; Michael Janssen; Britton Jeter; Wu Jiang; Michael D. Johnson; Taehyun Jung; Mansour Karami; Ramesh Karuppusamy; Mark Kettenis; Dong-Jin Kim; Jongsoo Kim; Junhan Kim; Jun Yi Koay; Patrick M. Koch; Shoko Koyama; Michael Kramer; Carsten Kramer; Tod R. Lauer; Aviad Levis; Yan-Rong Li; Zhiyuan Li; Michael Lindqvist; Rocco Lico; Greg Lindahl; Jun Liu; Kuo Liu; Elisabetta Liuzzo; Wen Ping Lo; Andrei Lobanov; Laurent Loinard; Colin J. Lonsdale; Nicholas R. MacDonald; Jirong Mao; Nicola Marchili; Daniel P. Marrone; Alan P. Marscher; Satoki Matsushita; Lynn D. Matthews; Lia Medeiros; Karl M. Menten; Izumi Mizuno; Yosuke Mizuno; James M. Moran; Kotaro Moriyama; Monika Moscibrodzka; Cornelia Müller; Gibwa Musoke; Alejandro Mus Mejías; Hiroshi Nagai; Neil M. Nagar; Masanori Nakamura; Ramesh Narayan; Gopal Narayanan; Iniyan Natarajan; Chunchong Ni; Aristeidis Noutsos; Hector Olivares; Gisela N. Ortiz-León; Feryal Özel; Daniel C. M. Palumbo; Ue-Li Pen; Dominic W. Pesce; Vincent Piétu; Richard Plambeck; Aleksandar Popstefanija; Oliver Porth; Felix M. Pötzl; Ben Prather; Jorge A. Preciado-López; Hung Yi Pu; Ramprasad Rao; Alexander W. Raymond; Luciano Rezzolla; Angelo Ricarte; Bart Ripperda; Freek Roelofs; Eduardo Ros; Mel Rose; Alan L. Roy; Chet Ruszczyk; Kazi L.J. Rygl; David Sánchez-Arguelles; Tuomas Savolainen; F. Peter Schloerb; Lijing Shao; Des Small; Bong Won Sohn; Jason SooHoo; He Sun; Fumie Tazaki; Alexandra J. Tetarenko; Paul Tiede; Remo P. J. Tilanus; Michael Titus; Kenji Toma; Pablo Torne; Tyler Trent; Efthalia Traianou; Sascha Trippe; Ilse van Bemmel; Huib Jan van Langevelde; Daniel R. van Rossum; Jan Wagner; Derek Ward-Thompson; Jonathan Weintroub; Norbert Wex; Robert Wharton; Maciek Wielgus; George N. Wong; Qingwen Wu; Doosoo Yoon; André Young; Ken Young; Ziri Younsi; Feng Yuan; Guang Yao Zhao; Shan Shan Zhao; M. Orienti; R. Adam; E. O. Angüner; C. Arcaro; C. Armand; Halim Ashkar; Michael Backes; V. Baghmanyan; V. Barbosa Martins; Monica Barnard; D. Berge; Konrad Bernlöhr; M. de Bony de Lavergne; Mischa Breuhaus; Tomasz Bulik; S. Caroff; A. Carosi; T. Chand; J. Devin; A. Djannati-Ataï; Axel Donath; Victor Doroshenko; Christopher J. Duffy; Sabrina Einecke; G. Fichet de Clairfontaine; Gilles Fontaine; Stefano Gabici; J. F. Glicenstein; Maria Haupt; G. Hermann; Jim Hinton; Clemens Hoischen; Tim Holch; Dieter Horns; Marek Jamrozy; Felix Jankowsky; V. Joshi; I. Jung-Richardt; U. Katz; Bruno Khelifi; Stefan Klepser; Nu. Komin; R. Konno; K. Kosack; Dmitriy Kostunin; Iryna Lypova; Jonathan Mackey; D. Malyshev; Paolo Marchegiani; A. Marcowith; G. Martí-Devesa; Manuel Meyer; Rafal Moderski; M. Mohamed; L. Mohrmann; E. Moulin; A. Nayerhoda; F. Niederwanger; Jacek Niemiec; L. Oakes; Stefan Ohm; R. D. Parsons; G. Peron; Q. Piel; A. Priyana Noel; Michael Punch; P. Reichherzer; A. Reimer; Olaf Reimer; L. Rinchiuso; E. Ruiz-Velasco; V. Sahakian; S. Sailer; Andrea Santangelo; M. Scalici; H. M. Schutte; M. Seglar-Arroyo; A. Sinha; Andreas Specovius; Christian Stegmann; T. Tavernier; Regis Terrier; Michelle Tsirou; C. van Eldik; B. van Soelen; Johannes Veh; Christo Venter; Heinrich J. Völk; Zorawar Wadiasingh; R. J. White; Yu Wun Wong; A. Yusafzai; M. Zacharias; Davit Zargaryan; A. A. Zdziarski; A. Zech; Sylvia Zhu; J. Zorn; Samuel Zouari; V. A. Acciari; L. A. Antonelli; A. Arbet Engels; Ana Babić; Andrés Baquero; J. A. Barrio; J. Becerra González; Wlodek Bednarek; Elisa Bernardini; A. Berti; Ciro Bigongiari; Oscar Blanch; Giacomo Bonnoli; Bošnjak; G. Busetto; Giovanni Ceribella; Matteo Cerruti; Ashot Chilingarian; Stefan Cikota; Sidika Merve Colak; E. Colombo; Jose Luis Contreras; Juan Cortina; Giacomo D'Amico; P. Da Vela; Francesco Dazzi; A. De Angelis; B. De Lotto; Jose Miguel Delgado; C. Delgado Mendez; D. Depaoli; F. Di Pierro; L. Di Venere; E. Do Souto Espiñeira; D. Dominis Prester; Alice Donini; Daniela Dorner; Michele Doro; Dominik Elsaesser; V. Fallah Ramazani; Alicia Fattorini; Giovanna Ferrara; M. V. Fonseca; Lluis Font; Satoshi Fukami; R. J. García López; M. Garczarczyk; M. Gaug; Nicola Giglietto; F. Giordano; Pawel Gliwny; Nikola Godinovic; Jarred Gershon Green; D. Hadasch; Alexander Hahn; Lea Heckmann; J. Herrera; John Hoang; Toshiaki Inada; Sanae Inoue; Kazuma Ishio; I. Jiménez; Jenni Jormanainen; M. Karjalainen; Daniel Kerszberg; J. Kushida; Damir Lelas; F. Leone; Elina Lindfors; Saverio Lombardi; Francesco Longo; R. López-Coto; Marcos López-Moya; A. López-Oramas; S. Loporchio; B. Machado de Oliveira Fraga; Camilla Maggio; Manuela Mallamaci; G. Maneva; Mosè Mariotti; Stefano Menchiari; Simone Mender; S. Mićanović; D. Miceli; R. Mirzoyan; E. Molina; Abelardo Moralejo; Daniel Morcuende; Victoria Moreno; E. Moretti; Cosimo Nigro; Koji Noda; S. Nozaki; Y. Ohtani; Tomohiko Oka; J. Otero-Santos; S. Paiano; M. Palatiello; J. M. Paredes; C. Perennes; Massimo Persic; P. G. Prada Moroni; Elisa Prandini; Chaitanya Priyadarshi; Ivica Puljak; Wolfgang Rhode; Marc Ribó; J. Rico; Chiara Righi; A. Rugliancich; Narek Sahakyan; Tomoki Saito; Francesco Gabriele Saturni; Kasper B. Schmidt; Julian Sitarek; I. Snidaric; Dorota Sobczyńska; Alessia Spolon; A. Stamerra; Y. Suda; P. Temnikov; Luca Tosti; Santiago Ubach; J. van Scherpenberg; M. Vazquez Acosta; S. Ventura; Vassil Verguilov; V. Vitale; I. Vovk; D. Zarić; Wystan Benbow; A. Brill; M. Capasso; M. K. Daniel; Manel Errando; Q. Feng; Lucy Fortson; Tarek M. Hassan; W. Jin; P. Kaaret; Gernot Maier; Reshmi Mukherjee; Daniel Nieto; S. Patel; M. Pohl; E. Pueschel; K. Ragan; Marcos Santander; Tomoya Hirota; Lang Cui; Kotaro Niinuma; Nobuyuki Sakai; Satoko Sawada-Satoh; Kiyoaki Wajima; Na Wang; Xiang Liu; Yoshinori Yonekura;doi: 10.3847/2041-8213/abef71 , 10.48550/arxiv.2104.06855 , 10.18452/26482 , 10.3204/pubdb-2021-02289
handle: https://repository.ubn.ru.nl/handle/2066/234240 , 11588/852706 , 2066/234240 , 1887/3273725 , 11370/ac0f3897-b9e9-4976-ae3e-b9bb0ff27cc2 , 10261/254872 , 11368/3029214 , 20.500.11769/528437 , 11589/254743 , 2318/1877411 , 11245.1/32dcb8b3-e7b9-4e76-b7e8-a1adeef9de28 , 21.11116/0000-0009-E122-2 , 21.11116/0000-0009-E124-0 , 11365/1147696
doi: 10.3847/2041-8213/abef71 , 10.48550/arxiv.2104.06855 , 10.18452/26482 , 10.3204/pubdb-2021-02289
handle: https://repository.ubn.ru.nl/handle/2066/234240 , 11588/852706 , 2066/234240 , 1887/3273725 , 11370/ac0f3897-b9e9-4976-ae3e-b9bb0ff27cc2 , 10261/254872 , 11368/3029214 , 20.500.11769/528437 , 11589/254743 , 2318/1877411 , 11245.1/32dcb8b3-e7b9-4e76-b7e8-a1adeef9de28 , 21.11116/0000-0009-E122-2 , 21.11116/0000-0009-E124-0 , 11365/1147696
Full list of authors: EHT MWL Science Working Group; Algaba, J. C.; Anczarski, J.; Asada, K.; Baloković, M.; Chandra, S.; Cui, Y. -Z.; Falcone, A. D.; Giroletti, M.; Goddi, C.; Hada, K.; Haggard, D.; Jorstad, S.; Kaur, A.; Kawashima, T.; Keating, G.; Kim, J. -Y.; Kino, M.; Komossa, S.; Kravchenko, E. V.; Krichbaum, T. P.; Lee, S. -S.; Lu, R. -S.; Lucchini, M.; Markoff, S.; Neilsen, J.; Nowak, M. A.; Park, J.; Principe, G.; Ramakrishnan, V.; Reynolds, M. T.; Sasada, M.; Savchenko, S. S.; Williamson, K. E.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Barrett, John; Bintley, Dan; Benson, Bradford A.; Blackburn, Lindy; Blundell, Raymond; Boland, Wilfred; Bouman, Katherine L.; Bower, Geoffrey C.; Boyce, Hope; Bremer, Michael; Brinkerink, Christiaan D.; Brissenden, Roger; Britzen, Silke; Broderick, Avery E.; Broguiere, Dominique; Bronzwaer, Thomas; Byun, Do-Young; Carlstrom, John E.; Chael, Andrew; Chan, Chi-Kwan; Chatterjee, Shami; Chatterjee, Koushik; Chen, Ming-Tang; Chen, Yongjun; Chesler, Paul M.; Cho, Ilje; Christian, Pierre; Conway, John E.; Cordes, James M.; Crawford, Thomas M.; Crew, Geoffrey B.; Cruz-Osorio, Alejandro; Davelaar, Jordy; de Laurentis, Mariafelicia; Deane, Roger; Dempsey, Jessica; Desvignes, Gregory; Dexter, Jason; Doeleman, Sheperd S.; Eatough, Ralph P.; Falcke, Heino; Farah, Joseph; Fish, Vincent L.; Fomalont, Ed; Ford, H. Alyson; Fraga-Encinas, Raquel; Friberg, Per; Fromm, Christian M.; Fuentes, Antonio; Galison, Peter; Gammie, Charles F.; García, Roberto; Gentaz, Olivier; Georgiev, Boris; Gold, Roman; Gómez, José L.; Gómez-Ruiz, Arturo I.; Gu, Minfeng; Gurwell, Mark; Hecht, Michael H.; Hesper, Ronald; Ho, Luis C.; Ho, Paul; Honma, Mareki; Huang, Chih-Wei L.; Huang, Lei; Hughes, David H.; Ikeda, Shiro; Inoue, Makoto; Issaoun, Sara; James, David J.; Jannuzi, Buell T.; Janssen, Michael; Jeter, Britton; Jiang, Wu; Jiménez-Rosales, Alejandra; Johnson, Michael D.; Jung, Taehyun; Karami, Mansour; Karuppusamy, Ramesh; Kettenis, Mark; Kim, Dong-Jin; Kim, Jongsoo; Kim, Junhan; Koay, Jun Yi; Kofuji, Yutaro; Koch, Patrick M.; Koyama, Shoko; Kramer, Michael; Kramer, Carsten; Kuo, Cheng-Yu; Lauer, Tod R.; Levis, Aviad; Li, Yan-Rong; Li, Zhiyuan; Lindqvist, Michael; Lico, Rocco; Lindahl, Greg; Liu, Jun; Liu, Kuo; Liuzzo, Elisabetta; Lo, Wen-Ping; Lobanov, Andrei P.; Loinard, Laurent; Lonsdale, Colin; MacDonald, Nicholas R.; Mao, Jirong; Marchili, Nicola; Marrone, Daniel P.; Marscher, Alan P.; Martí-Vidal, Iván; Matsushita, Satoki; Matthews, Lynn D.; Medeiros, Lia; Menten, Karl M.; Mizuno, Izumi; Mizuno, Yosuke; Moran, James M.; Moriyama, Kotaro; Moscibrodzka, Monika; Müller, Cornelia; Musoke, Gibwa; Mejías, Alejandro Mus; Nagai, Hiroshi; Nagar, Neil M.; Nakamura, Masanori; Narayan, Ramesh; Narayanan, Gopal; Natarajan, Iniyan; Nathanail, Antonios; Neri, Roberto; Ni, Chunchong; Noutsos, Aristeidis; Okino, Hiroki; Olivares, Héctor; Ortiz-León, Gisela N.; Oyama, Tomoaki; Özel, Feryal; Palumbo, Daniel C. M.; Patel, Nimesh; Pen, Ue-Li; Pesce, Dominic W.; Piétu, Vincent; Plambeck, Richard; Popstefanija, Aleksandar; Porth, Oliver; Pötzl, Felix M.; Prather, Ben; Preciado-López, Jorge A.; Psaltis, Dimitrios; Pu, Hung-Yi; Rao, Ramprasad; Rawlings, Mark G.; Raymond, Alexander W.; Rezzolla, Luciano; Ricarte, Angelo; Ripperda, Bart; Roelofs, Freek; Rogers, Alan; Ros, Eduardo; Rose, Mel; Roshanineshat, Arash; Rottmann, Helge; Roy, Alan L.; Ruszczyk, Chet; Rygl, Kazi L. J.; Sánchez, Salvador; Sánchez-Arguelles, David; Savolainen, Tuomas; Schloerb, F. Peter; Schuster, Karl-Friedrich; Shao, Lijing; Shen, Zhiqiang; Small, Des; Sohn, Bong Won; Soohoo, Jason; Sun, He; Tazaki, Fumie; Tetarenko, Alexandra J.; Tiede, Paul; Tilanus, Remo P. J.; Titus, Michael; Toma, Kenji; Torne, Pablo; Trent, Tyler; Traianou, Efthalia; Trippe, Sascha; van Bemmel, Ilse; van Langevelde, Huib Jan; van Rossum, Daniel R.; Wagner, Jan; Ward-Thompson, Derek; Wardle, John; Weintroub, Jonathan; Wex, Norbert; Wharton, Robert; Wielgus, Maciek; Wong, George N.; Wu, Qingwen; Yoon, Doosoo; Young, André; Young, Ken; Younsi, Ziri; Yuan, Feng; Yuan, Ye-Fei; Zensus, J. Anton; Zhao, Guang-Yao; Zhao, Shan-Shan; Fermi Large Area Telescope Collaboration; Principe, G.; Giroletti, M.; D'Ammando, F.; Orienti, M.; H. E. S. S. Collaboration; Abdalla, H.; Adam, R.; Aharonian, F.; Benkhali, F. Ait; Angüner, E. O.; Arcaro, C.; Armand, C.; Armstrong, T.; Ashkar, H.; Backes, M.; Baghmanyan, V.; Barbosa Martins, V.; Barnacka, A.; Barnard, M.; Becherini, Y.; Berge, D.; Bernlöhr, K.; Bi, B.; Böttcher, M.; Boisson, C.; Bolmont, J.; de Lavergne, M. De Bony; Breuhaus, M.; Brun, F.; Brun, P.; Bryan, M.; Büchele, M.; Bulik, T.; Bylund, T.; Caroff, S.; Carosi, A.; Casanova, S.; Chand, T.; Chen, A.; Cotter, G.; Curyło, M.; Damascene Mbarubucyeye, J.; Davids, I. D.; Davies, J.; Deil, C.; Devin, J.; Dewilt, P.; Dirson, L.; Djannati-Ataï, A.; Dmytriiev, A.; Donath, A.; Doroshenko, V.; Duffy, C.; Dyks, J.; Egberts, K.; Eichhorn, F.; Einecke, S.; Emery, G.; Ernenwein, J. -P.; Feijen, K.; Fegan, S.; Fiasson, A.; de Clairfontaine, G. Fichet; Fontaine, G.; Funk, S.; Füßling, M.; Gabici, S.; Gallant, Y. A.; Giavitto, G.; Giunti, L.; Glawion, D.; Glicenstein, J. F.; Gottschall, D.; Grondin, M. -H.; Hahn, J.; Haupt, M.; Hermann, G.; Hinton, J. A.; Hofmann, W.; Hoischen, C.; Holch, T. L.; Holler, M.; Hörbe, M.; Horns, D.; Huber, D.; Jamrozy, M.; Jankowsky, D.; Jankowsky, F.; Jardin-Blicq, A.; Joshi, V.; Jung-Richardt, I.; Kasai, E.; Kastendieck, M. A.; Katarzyński, K.; Katz, U.; Khangulyan, D.; Khélifi, B.; Klepser, S.; Kluźniak, W.; Komin, Nu.; Konno, R.; Kosack, K.; Kostunin, D.; Kreter, M.; Lamanna, G.; Lemière, A.; Lemoine-Goumard, M.; Lenain, J. -P.; Levy, C.; Lohse, T.; Lypova, I.; Mackey, J.; Majumdar, J.; Malyshev, D.; Malyshev, D.; Marandon, V.; Marchegiani, P.; Marcowith, A.; Mares, A.; Martí-Devesa, G.; Marx, R.; Maurin, G.; Meintjes, P. J.; Meyer, M.; Moderski, R.; Mohamed, M.; Mohrmann, L.; Montanari, A.; Moore, C.; Morris, P.; Moulin, E.; Muller, J.; Murach, T.; Nakashima, K.; Nayerhoda, A.; de Naurois, M.; Ndiyavala, H.; Niederwanger, F.; Niemiec, J.; Oakes, L.; O'Brien, P.; Odaka, H.; Ohm, S.; Olivera-Nieto, L.; de Ona Wilhelmi, E.; Ostrowski, M.; Panter, M.; Panny, S.; Parsons, R. D.; Peron, G.; Peyaud, B.; Piel, Q.; Pita, S.; Poireau, V.; Noel, A. Priyana; Prokhorov, D. A.; Prokoph, H.; Pühlhofer, G.; Punch, M.; Quirrenbach, A.; Rauth, R.; Reichherzer, P.; Reimer, A.; Reimer, O.; Remy, Q.; Renaud, M.; Rieger, F.; Rinchiuso, L.; Romoli, C.; Rowell, G.; Rudak, B.; Ruiz-Velasco, E.; Sahakian, V.; Sailer, S.; Sanchez, D. A.; Santangelo, A.; Sasaki, M.; Scalici, M.; Schutte, H. M.; Schwanke, U.; Schwemmer, S.; Seglar-Arroyo, M.; Senniappan, M.; Seyffert, A. S.; Shafi, N.; Shiningayamwe, K.; Simoni, R.; Sinha, A.; Sol, H.; Specovius, A.; Spencer, S.; Spir-Jacob, M.; Stawarz, Ł.; Sun, L.; Steenkamp, R.; Stegmann, C.; Steinmassl, S.; Steppa, C.; Takahashi, T.; Tavernier, T.; Taylor, A. M.; Terrier, R.; Tiziani, D.; Tluczykont, M.; Tomankova, L.; Trichard, C.; Tsirou, M.; Tuffs, R.; Uchiyama, Y.; van der Walt, D. J.; van Eldik, C.; van Rensburg, C.; van Soelen, B.; Vasileiadis, G.; Veh, J.; Venter, C.; Vincent, P.; Vink, J.; Völk, H. J.; Vuillaume, T.; Wadiasingh, Z.; Wagner, S. J.; Watson, J.; Werner, F.; White, R.; Wierzcholska, A.; Wong, Yu Wun; Yusafzai, A.; Zacharias, M.; Zanin, R.; Zargaryan, D.; Zdziarski, A. A.; Zech, A.; Zhu, S. J.; Zorn, J.; Zouari, S.; Żywucka, N.; MAGIC Collaboration; Acciari, V. A.; Ansoldi, S.; Antonelli, L. A.; Engels, A. Arbet; Artero, M.; Asano, K.; Baack, D.; Babić, A.; Baquero, A.; de Almeida, U. Barres; Barrio, J. A.; Becerra González, J.; Bednarek, W.; Bellizzi, L.; Bernardini, E.; Bernardos, M.; Berti, A.; Besenrieder, J.; Bhattacharyya, W.; Bigongiari, C.; Biland, A.; Blanch, O.; Bonnoli, G.; Bošnjak, Ž.; Busetto, G.; Carosi, R.; Ceribella, G.; Cerruti, M.; Chai, Y.; Chilingarian, A.; Cikota, S.; Colak, S. M.; Colombo, E.; Contreras, J. L.; Cortina, J.; Covino, S.; D'Amico, G.; D'Elia, V.; da Vela, P.; Dazzi, F.; de Angelis, A.; de Lotto, B.; Delfino, M.; Delgado, J.; Delgado Mendez, C.; Depaoli, D.; di Pierro, F.; di Venere, L.; Do Souto Espiñeira, E.; Dominis Prester, D.; Donini, A.; Dorner, D.; Doro, M.; Elsaesser, D.; Ramazani, V. Fallah; Fattorini, A.; Ferrara, G.; Fonseca, M. V.; Font, L.; Fruck, C.; Fukami, S.; García López, R. J.; Garczarczyk, M.; Gasparyan, S.; Gaug, M.; Giglietto, N.; Giordano, F.; Gliwny, P.; Godinović, N.; Green, J. G.; Green, D.; Hadasch, D.; Hahn, A.; Heckmann, L.; Herrera, J.; Hoang, J.; Hrupec, D.; Hütten, M.; Inada, T.; Inoue, S.; Ishio, K.; Iwamura, Y.; Jiménez, I.; Jormanainen, J.; Jouvin, L.; Kajiwara, Y.; Karjalainen, M.; Kerszberg, D.; Kobayashi, Y.; Kubo, H.; Kushida, J.; Lamastra, A.; Lelas, D.; Leone, F.; Lindfors, E.; Lombardi, S.; Longo, F.; López-Coto, R.; López-Moya, M.; López-Oramas, A.; Loporchio, S.; Machado de Oliveira Fraga, B.; Maggio, C.; Majumdar, P.; Makariev, M.; Mallamaci, M.; Maneva, G.; Manganaro, M.; Mannheim, K.; Maraschi, L.; Mariotti, M.; Martínez, M.; Mazin, D.; Menchiari, S.; Mender, S.; Mićanović, S.; Miceli, D.; Miener, T.; Minev, M.; Miranda, J. M.; Mirzoyan, R.; Molina, E.; Moralejo, A.; Morcuende, D.; Moreno, V.; Moretti, E.; Neustroev, V.; Nigro, C.; Nilsson, K.; Nishijima, K.; Noda, K.; Nozaki, S.; Ohtani, Y.; Oka, T.; Otero-Santos, J.; Paiano, S.; Palatiello, M.; Paneque, D.; Paoletti, R.; Paredes, J. M.; Pavletić, L.; Peñil, P.; Perennes, C.; Persic, M.; Moroni, P. G. Prada; Prandini, E.; Priyadarshi, C.; Puljak, I.; Rhode, W.; Ribó, M.; Rico, J.; Righi, C.; Rugliancich, A.; Saha, L.; Sahakyan, N.; Saito, T.; Sakurai, S.; Satalecka, K.; Saturni, F. G.; Schleicher, B.; Schmidt, K.; Schweizer, T.; Sitarek, J.; Šnidarić, I.; Sobczynska, D.; Spolon, A.; Stamerra, A.; Strom, D.; Strzys, M.; Suda, Y.; Surić, T.; Takahashi, M.; Tavecchio, F.; Temnikov, P.; Terzić, T.; Teshima, M.; Tosti, L.; Truzzi, S.; Tutone, A.; Ubach, S.; van Scherpenberg, J.; Vanzo, G.; Vazquez Acosta, M.; Ventura, S.; Verguilov, V.; Vigorito, C. F.; Vitale, V.; Vovk, I.; Will, M.; Wunderlich, C.; Zarić, D.; VERITAS Collaboration; Adams, C. B.; Benbow, W.; Brill, A.; Capasso, M.; Christiansen, J. L.; Chromey, A. J.; Daniel, M. K.; Errando, M.; Farrell, K. A.; Feng, Q.; Finley, J. P.; Fortson, L.; Furniss, A.; Gent, A.; Giuri, C.; Hassan, T.; Hervet, O.; Holder, J.; Hughes, G.; Humensky, T. B.; Jin, W.; Kaaret, P.; Kertzman, M.; Kieda, D.; Kumar, S.; Lang, M. J.; Lundy, M.; Maier, G.; Moriarty, P.; Mukherjee, R.; Nieto, D.; Nievas-Rosillo, M.; O'Brien, S.; Ong, R. A.; Otte, A. N.; Patel, S.; Pfrang, K.; Pohl, M.; Prado, R. R.; Pueschel, E.; Quinn, J.; Ragan, K.; Reynolds, P. T.; Ribeiro, D.; Richards, G. T.; Roache, E.; Rulten, C.; Ryan, J. L.; Santander, M.; Sembroski, G. H.; Shang, R.; Weinstein, A.; Williams, D. A.; Williamson, T. J.; Eavn Collaboration; Hirota, Tomoya; Cui, Lang; Niinuma, Kotaro; Ro, Hyunwook; Sakai, Nobuyuki; Sawada-Satoh, Satoko; Wajima, Kiyoaki; Wang, Na; Liu, Xiang; Yonekura, Yoshinori The financial support of the German BMBF, MPG and HGF; the Italian INFN and INAF; the Swiss National Fund SNF; the ERDF under the Spanish Ministerio de Ciencia e Innovacion (MICINN) (FPA2017-87859-P, FPA2017-85668-P, FPA2017- 82729-C6-5-R, FPA2017-90566-REDC, PID2019-104114RBC31, PID2019-104114RB-C32, PID2019-105510GB-C31,PID 2019-107847RB-C41, PID2019-107847RB-C42, PID2019- 107988GB-C22); the Indian Department of Atomic Energy; the Japanese ICRR, the University of Tokyo, JSPS, and MEXT; the Bulgarian Ministry of Education and Science, National RI Roadmap Project DO1-268/16.12.2019 and the Academy of Finland grant No. 320045 is gratefully acknowledged. This work was also supported by the Spanish Centro de Excelencia “Severo Ochoa” SEV-2016-0588 and CEX2019- 000920-S, and “Maria de Maeztu” CEX2019-000918-M, the Unidad de Excelencia “Maria de Maeztu” MDM-2015-0509- 18-2 and the “la Caixa” Foundation (fellowship LCF/BQ/ PI18/11630012) and by the CERCA program of the Generalitat de Catalunya; by the Croatian Science Foundation (HrZZ) Project IP-2016-06-9782 and the University of Rijeka Project 13.12.1.3.02; by the DFG Collaborative Research Centers SFB823/C4 and SFB876/C3; the Polish National Research Centre grant UMO-2016/22/M/ST9/00382; and by the Brazilian MCTIC, CNPq, and FAPERJ. This research is supported by grants from the U.S. Department of Energy Office of Science, the U.S. National Science Foundation and the Smithsonian Institution, by NSERC in Canada, and by the Helmholtz Association in Germany. This research used resources provided by the Open Science Grid, which is supported by the National Science Foundation and the U.S. Department of Energy’s Office of Science, and resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231. We acknowledge the excellent work of the technical support staff at the Fred Lawrence Whipple Observatory and at the collaborating institutions in the construction and operation of the instrument. In 2017, the Event Horizon Telescope (EHT) Collaboration succeeded in capturing the first direct image of the center of the M87 galaxy. The asymmetric ring morphology and size are consistent with theoretical expectations for a weakly accreting supermassive black hole of mass ∼6.5 × 109 M o˙. The EHTC also partnered with several international facilities in space and on the ground, to arrange an extensive, quasi-simultaneous multi-wavelength campaign. This Letter presents the results and analysis of this campaign, as well as the multi-wavelength data as a legacy data repository. We captured M87 in a historically low state, and the core flux dominates over HST-1 at high energies, making it possible to combine core flux constraints with the more spatially precise very long baseline interferometry data. We present the most complete simultaneous multi-wavelength spectrum of the active nucleus to date, and discuss the complexity and caveats of combining data from different spatial scales into one broadband spectrum. We apply two heuristic, isotropic leptonic single-zone models to provide insight into the basic source properties, but conclude that a structured jet is necessary to explain M87's spectrum. We can exclude that the simultaneous γ-ray emission is produced via inverse Compton emission in the same region producing the EHT mm-band emission, and further conclude that the γ-rays can only be produced in the inner jets (inward of HST-1) if there are strongly particle-dominated regions. Direct synchrotron emission from accelerated protons and secondaries cannot yet be excluded. Peer reviewed
NARCIS arrow_drop_down NARCIS; The Astrophysical Journal LettersArticle . 2021IRIS - Università degli Studi di Catania; METIS Research Information System; NARCIS; Archivio Istituzionale della Ricerca - Politecnico di Bari; Archivio Istituzionale; The Astrophysical Journal Letters; Archivio della ricerca - Università degli studi di Napoli Federico II; Croatian Scientific Bibliography - CROSBIOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYData sources: European Union Open Data Portal; Sygma; IRIS - Università degli Studi di Catania; Crossref; METIS Research Information System; NARCIS; Archivio Istituzionale della Ricerca - Politecnico di Bari; Archivio Istituzionale; Archivio della ricerca - Università degli studi di Napoli Federico II; Croatian Scientific Bibliography - CROSBICORE (RIOXX-UK Aggregator)Article . 2021License: CC BYFull-Text: https://clok.uclan.ac.uk/37450/1/pdf.pdfData sources: CORE (RIOXX-UK Aggregator)University of Southern Denmark Research OutputArticle . 2021Data sources: University of Southern Denmark Research OutputThe Astrophysical Journal LettersArticle . 2021Data sources: University of Southern Denmark Research Outputedoc-Server. Open-Access-Publikationsserver der Humboldt-Universität zu BerlinArticle . 2021 . Peer-reviewedUniversity of Oulu Repository - JultikaArticle . 2021Data sources: University of Oulu Repository - JultikaOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2021Data sources: OA@INAF - Istituto Nazionale di AstrofisicaIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedAaltodoc Publication ArchiveArticle . 2021 . Peer-reviewedData sources: Aaltodoc Publication ArchiveLeiden University Scholarly Publications RepositoryOther literature type . 2021License: CC BYData sources: Leiden University Scholarly Publications RepositoryArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Archivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di Pisaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 54 citations 54 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!visibility 158visibility views 158 download downloads 335 Powered bymore_vert NARCIS arrow_drop_down NARCIS; The Astrophysical Journal LettersArticle . 2021IRIS - Università degli Studi di Catania; METIS Research Information System; NARCIS; Archivio Istituzionale della Ricerca - Politecnico di Bari; Archivio Istituzionale; The Astrophysical Journal Letters; Archivio della ricerca - Università degli studi di Napoli Federico II; Croatian Scientific Bibliography - CROSBIOther literature type . Article . 2021 . Peer-reviewedLicense: CC BYData sources: European Union Open Data Portal; Sygma; IRIS - Università degli Studi di Catania; Crossref; METIS Research Information System; NARCIS; Archivio Istituzionale della Ricerca - Politecnico di Bari; Archivio Istituzionale; Archivio della ricerca - Università degli studi di Napoli Federico II; Croatian Scientific Bibliography - CROSBICORE (RIOXX-UK Aggregator)Article . 2021License: CC BYFull-Text: https://clok.uclan.ac.uk/37450/1/pdf.pdfData sources: CORE (RIOXX-UK Aggregator)University of Southern Denmark Research OutputArticle . 2021Data sources: University of Southern Denmark Research OutputThe Astrophysical Journal LettersArticle . 2021Data sources: University of Southern Denmark Research Outputedoc-Server. Open-Access-Publikationsserver der Humboldt-Universität zu BerlinArticle . 2021 . Peer-reviewedUniversity of Oulu Repository - JultikaArticle . 2021Data sources: University of Oulu Repository - JultikaOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2021Data sources: OA@INAF - Istituto Nazionale di AstrofisicaIRIS - Università degli Studi di CataniaArticle . 2021Data sources: IRIS - Università degli Studi di CataniaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedAaltodoc Publication ArchiveArticle . 2021 . Peer-reviewedData sources: Aaltodoc Publication ArchiveLeiden University Scholarly Publications RepositoryOther literature type . 2021License: CC BYData sources: Leiden University Scholarly Publications RepositoryArchivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Archivio della Ricerca - Università di PisaArticle . 2021Data sources: Archivio della Ricerca - Università di Pisaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2021 Italy, FrancePublisher:Elsevier BV Publicly fundedFunded by:NSF | WoU-MMA:Astrophysics with..., NSF | Collaborative Research: M..., NSF | TeV Astrophysics with the... +9 projectsNSF| WoU-MMA:Astrophysics with a New Very-High-Energy Gamma-Ray Telescope ,NSF| Collaborative Research: MRI Consortium: Development of a Novel Telescope for Very High-Energy Gamma-Ray Astrophysics ,NSF| TeV Astrophysics with the VERITAS Gamma Ray Observatory ,NSF| Collaborative Research: MRI Consortium: Development of a Novel Telescope for Very High-Energy Gamma-Ray Astrophysics ,NSF| Particle and Gamma-Ray Astrophysics with HAWC/VERITAS (Utah Group Grant) ,NSF| Wou-MMA: Particle Astrophysics with VERITAS and CTA ,NSF| WoU-MMA: Operations of VERITAS in the Epoch 2019 to 2022 ,NSF| Gamma-Ray Astronomy and Cosmic-ray Astrophysics with the VERITAS and HAWC Observatories (University of Utah Group) ,NSF| Collaborative Research: MRI Consortium: Development of a Novel Telescope for Very High-Energy Gamma-Ray Astrophysics ,NSF| Astrophysics with Very-High-Energy Gamma Rays ,NSF| Multi-Messenger Astrophysics with the Cherenkov Telescope Array ,NSF| Astroparticle Physics with the VERITAS and CTA Gamma-Ray ObservatoriesC. B. Adams; Ruben Alfaro; G. Ambrosi; M. Ambrosio; Carla Aramo; T. C. Arlen; P. I. Batista; Wystan Benbow; B. Bertucci; Elisabetta Bissaldi; Jonathan Biteau; M. Bitossi; A. Boiano; C. Bonavolontà; Richard Bose; A. Bouvier; A. Brill; A. M. Brown; J. H. Buckley; Karen Byrum; R. A. Cameron; Rodolfo Canestrari; M. Capasso; M. Caprai; Corbin Covault; D. Depaoli; Manel Errando; S. J. Fegan; Q. Feng; E. Fiandrini; G. M. Foote; P. Fortin; Stefan Funk; Amy Furniss; Fernando Garfias; Alasdair E. Gent; Nicola Giglietto; Francesco Giordano; Enrico Giro; Maria Magdalena González; V. J. Guarino; R. Halliday; Olivier Hervet; Jamie Holder; G. Hughes; T. B. Humensky; Maria Ionica; Arturo Iriarte; W. Jin; C. A. Johnson; P. Kaaret; David Kieda; B. Kim; A. Kuznetsov; Jonathan S. Lapington; F. Licciulli; S. Loporchio; V. Masone; K. Meagher; Thomas Meures; B. A. W. Mode; S. I. Mognet; Reshmi Mukherjee; T. Nguyen; Daniel Nieto; Akira Okumura; N. Otte; N. La Palombara; F. R. Pantaleo; Riccardo Paoletti; G. Pareschi; A. Petrashyk; F. Di Pierro; E. Pueschel; P. T. Reynolds; D. Ribeiro; Gordon T. Richards; E. Roache; D. Ross; Julien Rousselle; Andrea Rugliancich; J. Ruíz-Díaz-Soto; Marcos Santander; S. Schlenstedt; Michael Schneider; Salvo Scuderi; R. Shang; G. Sironi; B. Stevenson; L. Stiaccini; Hiroyasu Tajima; L. P. Taylor; J. Thornhill; L. Tosti; Gagik Tovmassian; V. Vagelli; M. Valentino; Justin Vandenbroucke; Vladimir Vassiliev; L. Di Venere; S. P. Wakely; Jason John Watson; R. J. White; P. Wilcox; David A. Williams; Matthew Wood; P. Yu; A. Zink;The Schwarzschild-Couder Telescope (SCT) is a telescope concept proposed for the Cherenkov Telescope Array. It employs a dual-mirror optical design to remove comatic aberrations over an $8^{\circ}$ field of view, and a high-density silicon photomultiplier camera (with a pixel resolution of 4 arcmin) to record Cherenkov emission from cosmic ray and gamma-ray initiated particle cascades in the atmosphere. The prototype SCT (pSCT), comprising a 9.7 m diameter primary mirror and a partially instrumented camera with 1536 pixels, has been constructed at the Fred Lawrence Whipple Observatory. The telescope was inaugurated in January 2019, with commissioning continuing throughout 2019. We describe the first campaign of observations with the pSCT, conducted in January and February of 2020, and demonstrate the detection of gamma-ray emission from the Crab Nebula with a statistical significance of $8.6\sigma$. Comment: 13 pages, 12 figures, 3 tables, submitted to Astroparticle Physics
Archivio Istituziona... arrow_drop_down Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 15 citations 15 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!more_vert Archivio Istituziona... arrow_drop_down Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021Archivio Istituzionale della Ricerca - Politecnico di BariArticle . 2021https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1016/j.astropartphys.2021.102562&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 France, IrelandPublisher:Cambridge University Press (CUP) Publicly fundedFunded by:SFI | Nonlinear wave-current in...SFI| Nonlinear wave-current interactions in the nearshore: addressing the role of vorticity and nonlinearity in the modelling of ocean energyAuthors: Didier Clamond; David Henry;Didier Clamond; David Henry;handle: 10468/12188
International audience; The aim of this note is to examine the efficacy of a recently developed approach to the recovery of nonlinear water waves from pressure measurements at the seabed, by applying it to the celebrated extreme Stokes wave.
Cork Open Research A... arrow_drop_down Cork Open Research Archive (CORA)Article . 2020License: CC BY NC NDData sources: Cork Open Research Archive (CORA)Journal of Fluid MechanicsArticle . 2020 . Peer-reviewedLicense: Cambridge Core User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Full-Text: https://hal.science/hal-02638111/documenthttps://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1017/jfm.2020.729&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Cork Open Research A... arrow_drop_down Cork Open Research Archive (CORA)Article . 2020License: CC BY NC NDData sources: Cork Open Research Archive (CORA)Journal of Fluid MechanicsArticle . 2020 . Peer-reviewedLicense: Cambridge Core User AgreementData sources: CrossrefMémoires en Sciences de l'Information et de la CommunicationArticle . 2020Full-Text: https://hal.science/hal-02638111/documenthttps://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1017/jfm.2020.729&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 United States, FrancePublisher:American Physical Society (APS) Publicly fundedFunded by:NSF | Gravitational Radiation a..., NSF | Maximizing Science Output..., UKRI | Friction Stir Welding Cra... +3 projectsNSF| Gravitational Radiation and Relativistic Astrophysics ,NSF| Maximizing Science Output of LIGO: Improved Detectors and Data Analysis ,UKRI| Friction Stir Welding Crawler for Internal Repair and Refurbishment of Pipelines - FSWBot ,EC| FunFiCO ,EC| BinGraSp ,UKRI| The Lancaster, Manchester, Sheffield Consortium for Fundamental Physics: Particle Physics from the LHC to the UniverseSarp Akcay; Sam R. Dolan; Chris Kavanagh; Jordan Moxon; Niels Warburton; Barry Wardell;We present the gravitational-wave flux balance law in an extreme mass-ratio binary with a spinning secondary. This law relates the flux of energy (angular momentum) radiated to null infinity and through the event horizon to the local change in the secondary's orbital energy (angular momentum) for generic (non-resonant) bound orbits in Kerr spacetime. As an explicit example we compute these quantities for a spin-aligned body moving on a circular orbit around a Schwarzschild black hole. We perform this calculation both analytically, via a high-order post-Newtonian expansion, and numerically in two different gauges. Using these results we demonstrate explicitly that our new balance law holds. Comment: Minor typos corrected
Caltech Authors arrow_drop_down https://doi.org/10.1103/physre...Article . 2020 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . Preprint . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.102.064013&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen 14 citations 14 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 4visibility views 4 download downloads 19 Powered bymore_vert Caltech Authors arrow_drop_down https://doi.org/10.1103/physre...Article . 2020 . Peer-reviewedLicense: APS Licenses for Journal Article Re-useData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: DataciteHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . Preprint . 2020add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevd.102.064013&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Other literature type , Preprint , Article 2020 France, Spain, Spain, FinlandPublisher:Copernicus GmbH Publicly fundedFunded by:UKRI | IFS-NET: Insect Food Secu..., EC | ACTRIS-2UKRI| IFS-NET: Insect Food Security NETwork ,EC| ACTRIS-2A. Cuesta-Mosquera; G. Močnik; G. Močnik; G. Močnik; L. Drinovec; L. Drinovec; L. Drinovec; T. Müller; S. Pfeifer; M. C. Minguillón; B. Briel; P. Buckley; V. Dudoitis; J. Fernández-García; M. Fernández-Amado; J. Ferreira De Brito; V. Riffault; H. Flentje; E. Heffernan; N. Kalivitis; A.-C. Kalogridis; H. Keernik; H. Keernik; L. Marmureanu; K. Luoma; A. Marinoni; M. Pikridas; G. Schauer; N. Serfozo; H. Servomaa; G. Titos; J. Yus-Díez; J. Yus-Díez; N. Zioła; A. Wiedensohler;handle: 10261/242385 , 2183/28139
Aerosolized black carbon is monitored worldwide to quantify its impact on air quality and climate. Given its importance, measurements of black carbon mass concentrations must be conducted with instruments operating in quality-checked and ensured conditions to generate data which are reliable and comparable temporally and geographically. In this study, we report the results from the largest characterization and intercomparison of filter-based absorption photometers, the Aethalometer model AE33, belonging to several European monitoring networks. Under controlled laboratory conditions, a total of 23 instruments measured mass concentrations of black carbon from three well-characterized aerosol sources: synthetic soot, nigrosin particles, and ambient air from the urban background of Leipzig, Germany. The objective was to investigate the individual performance of the instruments and their comparability; we analyzed the response of the instruments to the different aerosol sources and the impact caused by the use of obsolete filter materials and the application of maintenance activities. Differences in the instrument-to-instrument variabilities from equivalent black carbon (eBC) concentrations reported at 880 nm were determined before maintenance activities (for soot measurements, average deviation from total least square regression was −2.0 % and the range −16 % to 7 %; for nigrosin measurements, average deviation was 0.4 % and the range −15 % to 17 %), and after they were carried out (for soot measurements, average deviation was −1.0 % and the range −14 % to 8 %; for nigrosin measurements, the average deviation was 0.5 % and the range −12 % to 15 %). The deviations are in most of the cases explained by the type of filter material employed by the instruments, the total particle load on the filter, and the flow calibration. The results of this intercomparison activity show that relatively small unit-to-unit variability of AE33-based particle light absorbing measurements is possible with well-maintained instruments. It is crucial to follow the guidelines for maintenance activities and the use of the proper filter tape in the AE33 to ensure high quality and comparable black carbon (BC) measurements among international observational networks. ACTRIS and COLOSSAL provided financial support for the execution of the experiments. Instrument S04-00387 is operated and maintained thanks to the Spanish Ministry of Science and Innovation (project nos. CGL2016-81092-R, CGL2017-42 90884REDT, and RTI2018.101154.A.I00). Gloria Titos is funded by the Juan de la Cierva-Incorporación postdoctoral program (grant no. IJCI-2016-29838). IMT Lille Douai (Joel Ferreira De Brito, Veronique Riffault) received financial support from the Labex CaPPA project, which is funded by the French National Research Agency (ANR) through the PIA (Programme d'Investissement d'Avenir) (contract no. ANR-11-LABX-0005-01), and the CLIMIBIO project; both projects are financed by the Regional Council “Hauts-de-France” and the European Regional Development Fund (ERDF). The operation of instruments S00-00055 and S02-00156 is funded by the projects CRISOL (MINECO/AEI/FEDER, UE; grant no. CGL2017-85344-R) and TIGAS-CM (grant no. Y2018/EMT-5177). Peer reviewed
Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2021License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAAtmospheric Measurement Techniques (AMT)Other literature type . 2021Data sources: Copernicus Publicationshttps://doi.org/10.5194/amt-20...Preprint . 2020 . Peer-reviewedLicense: CC BYData sources: CrossrefRepositorio da Universidade da CoruñaArticle . 2021License: CC BYData sources: Repositorio da Universidade da CoruñaRecolector de Ciencia Abierta, RECOLECTA; Atmospheric Measurement TechniquesArticle . 2021 . Peer-reviewedLicense: CC BYHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiAtmospheric Measurement Techniques (AMT)Other literature type . 2020Data sources: Copernicus PublicationsRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/amt-2020-344&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 21 citations 21 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 25visibility views 25 download downloads 68 Powered bymore_vert Recolector de Cienci... arrow_drop_down Recolector de Ciencia Abierta, RECOLECTAArticle . 2021License: CC BYData sources: Recolector de Ciencia Abierta, RECOLECTAAtmospheric Measurement Techniques (AMT)Other literature type . 2021Data sources: Copernicus Publicationshttps://doi.org/10.5194/amt-20...Preprint . 2020 . Peer-reviewedLicense: CC BYData sources: CrossrefRepositorio da Universidade da CoruñaArticle . 2021License: CC BYData sources: Repositorio da Universidade da CoruñaRecolector de Ciencia Abierta, RECOLECTA; Atmospheric Measurement TechniquesArticle . 2021 . Peer-reviewedLicense: CC BYHELDA - Digital Repository of the University of HelsinkiArticle . 2021 . Peer-reviewedData sources: HELDA - Digital Repository of the University of HelsinkiAtmospheric Measurement Techniques (AMT)Other literature type . 2020Data sources: Copernicus PublicationsRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2021 . Peer-reviewedadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/amt-2020-344&type=result"></script>'); --> </script>
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